@article{oke_absolute_1974,
	title = {Absolute {Spectral} {Energy} {Distributions} for {White} {Dwarfs}},
	volume = {27},
	issn = {0067-0049},
	url = {http://adsabs.harvard.edu/abs/1974ApJS...27...21O},
	doi = {10.1086/190287},
	abstract = {Abstract image available at: 
http://adsabs.harvard.edu/abs/1974ApJS...27...21O},
	urldate = {2018-10-23},
	journal = {ApJS},
	author = {Oke, J. B.},
	month = feb,
	year = {1974},
	pages = {21}
}

@ARTICLE{Crain15_eagle,
       author = {{Crain}, Robert A. and {Schaye}, Joop and {Bower}, Richard G. and {Furlong}, Michelle and {Schaller}, Matthieu and {Theuns}, Tom and {Dalla Vecchia}, Claudio and {Frenk}, Carlos S. and {McCarthy}, Ian G. and {Helly}, John C. and {Jenkins}, Adrian and {Rosas-Guevara}, Yetli M. and {White}, Simon D.~M. and {Trayford}, James W.},
        title = "{The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: haloes, cosmology: theory, Astrophysics - Astrophysics of Galaxies},
         year = 2015,
        month = jun,
       volume = {450},
       number = {2},
        pages = {1937-1961},
          doi = {10.1093/mnras/stv725},
archivePrefix = {arXiv},
       eprint = {1501.01311},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015MNRAS.450.1937C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@article{Willott2015,
abstract = {We present Atacama Large Millimeter Array (ALMA) detections of atomic carbon line and dust continuum emission in two UV-luminous galaxies at redshift 6. The far-infrared (FIR) luminosities of these galaxies are substantially lower than similar starbursts at later cosmic epochs, indicating an evolution in the dust properties with redshift, in agreement with the evolution seen in ultraviolet (UV) attenuation by dust. The [CII] to FIR ratios are found to be higher than at low redshift showing that [CII] should be readily detectable by ALMA within the reionization epoch. One of the two galaxies shows a complex merger nature with the less massive component dominating the UV emission and the more massive component dominating the FIR line and continuum. Using the interstellar atomic carbon line to derive the systemic redshifts we investigate the velocity of Lyman alpha emission emerging from high-z galaxies. In contrast to previous work, we find no evidence for decreasing Lyman alpha velocity shifts at high-redshift. We observe an increase in velocity shifts from z$\sim$ 2 to z$\sim$6, consistent with the effects of increased IGM absorption.},
archivePrefix = {arXiv},
arxivId = {1504.05875},
author = {Willott, Chris J. and Carilli, Chris L. and Wagg, Jeff and Wang, Ran},
eprint = {1504.05875},
keywords = {ALMA,dust,high-z},
mendeley-tags = {ALMA,dust,high-z},
month = {apr},
pages = {10},
title = {{Star formation and the interstellar medium in z>6 UV-luminous Lyman-break galaxies}},
url = {http://arxiv.org/abs/1504.05875},
year = {2015}
}
@article{Bowler2014a,
abstract = {We present the results of a new search for bright star-forming galaxies at redshift z $\sim$= 7 within the UltraVISTA second data release (DR2) and UKIDSS (UKIRT Infrared Deep Sky Survey) UDS (Ultra Deep Survey) DR10 data, which together provide 1.65 deg2 of near-infrared imaging with overlapping optical and Spitzer data. Using a full photometric redshift analysis, to identify high-redshift galaxies and reject contaminants, we have selected a sample of 34 luminous (-22.7&lt;M_{UV}&lt;-21.2) galaxies with 6.5 &lt; z &lt; 7.5. Crucially, the deeper imaging provided by UltraVISTA DR2 confirms all of the robust objects previously uncovered by Bowler et al., validating our selection technique. Our new expanded galaxy sample includes the most massive galaxies known at z $\sim$= 7, with M* $\sim$= 1010 M&amp;sun;, and the majority are resolved, consistent with larger sizes (r1/2 $\sim$= 1-1.5 kpc) than displayed by less massive galaxies. From our final robust sample, we determine the form of the bright end of the rest-frame UV galaxy luminosity function (LF) at z $\sim$= 7, providing strong evidence that it does not decline as steeply as predicted by the Schechter-function fit to fainter data. We exclude the possibility that this is due to either gravitational lensing, or significant contamination of our galaxy sample by active galactic nuclei (AGN). Rather, our results favour a double power-law form for the galaxy LF at high redshift, or, more interestingly, an LF which simply follows the form of the dark matter halo mass function at bright magnitudes. This suggests that the physical mechanism which inhibits star formation activity in massive galaxies (i.e. AGN feedback or some other form of `mass quenching') has yet to impact on the observable galaxy LF at z $\sim$= 7, a conclusion supported by the estimated masses of our brightest galaxies which have only just reached a mass comparable to the critical `quenching mass' of M* $\sim$= 1010.2 M&amp;sun; derived from studies of the mass function of star-forming galaxies at lower redshift.},
author = {Bowler, R. A. A. and Dunlop, J. S. and McLure, R. J. and Rogers, A. B. and McCracken, H. J. and Milvang-Jensen, B. and Furusawa, H. and Fynbo, J. P. U. and Taniguchi, Y. and Afonso, J. and Bremer, M. N. and {Le Fevre}, O.},
doi = {10.1093/mnras/stu449},
issn = {0035-8711},
journal = {Monthly Notices of the Royal Astronomical Society},
keywords = {galaxies: evolution,galaxies: formation,galaxies: high-redshift,high-z},
mendeley-tags = {high-z},
month = {apr},
number = {3},
pages = {2810--2842},
title = {{The bright end of the galaxy luminosity function at z =7: before the onset of mass quenching?}},
url = {http://adsabs.harvard.edu/abs/2014MNRAS.440.2810B},
volume = {440},
year = {2014}
}
@article{Stefanon2015,
abstract = {We study the population of massive (i.e., $\log(M_*/M_\odot)>11$) galaxies at $4<z<7$ using a Spitzer IRAC complete sample obtained complementing the $K_\mathrm{s}$-band selected UltraVISTA catalog with detections in IRAC. Using this catalog we investigate, for the first time, the evolution of the massive end of the stellar mass functions at $4<z<7$. We consider the systematic effects of introducing a bayesian prior in the measurements of the photometric redshift as well as of different star formation histories (SFHs) and of nebular emission lines in the recovery of stellar population parameters. We show that our results are most affected by the bayesian prior, while nebular emission lines and SFHs only introduce a small dispersion in the measurements. Given the rarity of very massive galaxies in the early universe, major contributions to the total error budget come from cosmic variance and poisson noise. The stellar mass functions (SMFs) obtained without the introduction of the bayesian prior do not show any evolution from $z\sim6.5$ to $z\sim 3.5$, suggesting that massive galaxies could already be present when the Universe was $\sim0.9$ Gyr old. However, the introduction of the bayesian prior reduced the number of $z>4$ galaxies with best fit masses $\log(M_*/M_\odot)>11$ by 83% implying a rapid growth of very massive galaxies in the first 1.5 Gyr of cosmic history. From the stellar-mass complete sample, we identify one candidate of a very massive ($\log(M_*/M_\odot)\sim11.5$), quiescent galaxy at $z\sim5.4$, with MIPS $24\mu$m detection suggesting the presence of a powerful obscured AGN. Finally, we show that the number of massive galaxies at $4<z<7$ measured in this work matches the number of massive galaxies at $3<z<6$ predicted by current models of galaxy formation.},
archivePrefix = {arXiv},
arxivId = {1408.3416},
author = {Stefanon, Mauro and Marchesini, Danilo and Muzzin, Adam and Brammer, Gabriel G. and Dunlop, James S. and Franx, Marijin and Fynbo, Johan P. U. and Labbe, Ivo and Milvang-Jensen, Bo and van Dokkum, Pieter G.},
eprint = {1408.3416},
file = {:Users/idavidzon/Astro/all_papers/Stefanon et al. - 2015.pdf:pdf;:Users/idavidzon/Astro/all_papers/Stefanon et al. - 2015(2).pdf:pdf},
journal = {\apj},
keywords = {GSMF,high-z,massive galaxies},
mendeley-tags = {GSMF,high-z,massive galaxies},
month = {aug},
number = {11},
pages = {23},
title = {{Stellar mass functions of galaxies at 4<z<7 from an IRAC-selected sample in COSMOS/UltraVISTA: limits on the abundance of very massive galaxies}},
url = {http://arxiv.org/abs/1408.3416},
volume = {803},
year = {2015}
}
@article{Wilkins2014,
abstract = {The sensitivity available to near-infrared surveys has recently allowed us to probe the galaxy population at z ≈ 7 and beyond. The existing Hubble Wide Field Camera 3 (WFC3) and Visible and Infrared Survey Telescope for Astronomy (VISTA) Infrared Camera (VIRCam) instruments allow deep surveys to be undertaken well beyond 1 mum - a capability that will be further extended with the launch and commissioning of the James Webb Space Telescope (JWST). As new regions of parameter space in both colour and depth are probed, new challenges for distant galaxy surveys are identified. In this paper, we present an analysis of the colours of L- and T-dwarf stars in widely used photometric systems. We also consider the implications of the newly identified Y-dwarf population - stars that are still cooler and less massive than T-dwarfs for both the photometric selection and spectroscopic follow-up of faint and distant galaxies. We highlight the dangers of working in the low-signal-to-noise regime, and the potential contamination of existing and future samples. We find that Hubble/WFC3 and VISTA/VIRCam Y-drop selections targeting galaxies at z ˜ 7.5 are vulnerable to contamination from T- and Y-class stars. Future observations using JWST, targeting the z ˜ 7 galaxy population, are also likely to prove difficult without deep medium-band observations. We demonstrate that single emission line detections in typical low-signal-to-noise spectroscopic observations may also be suspect, due to the unusual spectral characteristics of the cool dwarf star population.},
annote = {http://pono.ucsd.edu/$\sim$adam/browndwarfs/spexprism},
author = {Wilkins, S. M. and Stanway, E. R. and Bremer, M. N.},
doi = {10.1093/mnras/stu029},
file = {:Users/idavidzon/Astro/all_papers/Wilkins, Stanway, Bremer - 2014.pdf:pdf},
issn = {0035-8711},
journal = {\mnras},
keywords = {brown dwarf,brown dwarfs,galaxies: evolution,galaxies: formation,galaxies: high-redshift,galaxies: starburst,ultraviolet: galaxies},
mendeley-tags = {brown dwarf},
month = {feb},
number = {1},
pages = {1038--1050},
title = {{High-redshift galaxies and low-mass stars}},
url = {http://adsabs.harvard.edu/abs/2014MNRAS.439.1038W},
volume = {439},
year = {2014}
}
@article{Grazian2015,
abstract = {Context. The form and evolution of the galaxy stellar mass function (GSMF) at high redshifts provide crucial information on star formation history and mass assembly in the young Universe, close or even prior to the epoch of reionization. Aims: We used the unique combination of deep optical/near-infrared/mid-infrared imaging provided by HST, Spitzer, and the VLT in the CANDELS-UDS, GOODS-South, and HUDF fields to determine the GSMF over the redshift range 3.5 <= z <= 7.5. Methods: We used the HST WFC3/IR near-infrared imaging from CANDELS and HUDF09, reaching H $\sim$= 27 - 28.5 over a total area of 369 arcmin2, in combination with associated deep HST ACS optical data, deep Spitzer IRAC imaging from the SEDS programme, and deep Y and K-band VLT Hawk-I images from the HUGS programme, to select a galaxy sample with high-quality photometric redshifts. These have been calibrated with more than 150 spectroscopic redshifts in the range 3.5 <= z <= 7.5, resulting in an overall precision of sigmaz/ (1 + z) $\sim$ 0.037. With this database we have determined the low-mass end of the high-redshift GSMF with unprecedented precision, reaching down to masses as low as M* $\sim$ 109 M&sun; at z = 4 and $\sim$6 × 109 M&sun; at z = 7. Results: We find that the GSMF at 3.5 <= z <= 7.5 depends only slightly on the recipes adopted to measure the stellar masses, namely the photometric redshifts, the star formation histories, the nebular contribution, or the presence of AGN in the parent sample. The low-mass end of the GSMF is steeper than has been found at lower redshifts, but appears to be unchanged over the redshift range probed here. Meanwhile the high-mass end of the GSMF appears to evolve primarily in density, although there is also some evidence of evolution in characteristic mass. Our results are very different from previous mass function estimates based on converting UV galaxy luminosity functions into mass functions via tight mass-to-light relations. Integrating our evolving GSMF over mass, we find that the growth of stellar mass density is barely consistent with the time-integral of the star formation rate density over cosmic time at z> 4. Conclusions: These results confirm the unique synergy of the CANDELS+HUDF, HUGS, and SEDS surveys for the discovery and study of moderate/low-mass galaxies at high redshifts, and reaffirm the importance of space-based infrared selection for the unbiased measurement of the evolving GSMF in the young Universe. Appendices are available in electronic form at http://www.aanda.org},
author = {Grazian, A. and Fontana, A. and Santini, P. and Dunlop, J. S. and Ferguson, H. C. and Castellano, M. and Amorin, R. and Ashby, M. L. N. and Barro, G. and Behroozi, P. and Boutsia, K. and Caputi, K. I. and Chary, R. R. and Dekel, A. and Dickinson, M. E. and Faber, S. M. and Fazio, G. G. and Finkelstein, S. L. and Galametz, A. and Giallongo, E. and Giavalisco, M. and Grogin, N. A. and Guo, Y. and Kocevski, D. and Koekemoer, A. M. and Koo, D. C. and Lee, K.-S. and Lu, Y. and Merlin, E. and Mobasher, B. and Nonino, M. and Papovich, C. and Paris, D. and Pentericci, L. and Reddy, N. and Renzini, A. and Salmon, B. and Salvato, M. and Sommariva, V. and Song, M. and Vanzella, E.},
doi = {10.1051/0004-6361/201424750},
file = {:Users/idavidzon/Astro/all_papers/Grazian et al. - 2015.pdf:pdf},
issn = {0004-6361},
journal = {\aap},
keywords = {GSMF,galaxies: distances and redshifts,galaxies: evolution,galaxies: high-redshift,galaxies: luminosity function,high-z,mass function},
mendeley-tags = {GSMF,high-z},
month = {mar},
pages = {A96},
title = {{The galaxy stellar mass function at 3.5 ≤ z ≤ 7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields}},
url = {http://adsabs.harvard.edu/abs/2015A%26A...575A..96G},
volume = {575},
year = {2015}
}
@article{Santini2012,
archivePrefix = {arXiv},
arxivId = {astro-ph.CO/1111.5728},
author = {Santini, P and Fontana, A and Grazian, A and Salimbeni, S and Fontanot, F and Paris, D and Boutsia, K and Castellano, M and Fiore, F and Gallozzi, S and Giallongo, E and Koekemoer, A.$\sim$M. and Menci, N and Pentericci, L and Somerville, R.$\sim$S.},
doi = {10.1051/0004-6361/201117513},
eprint = {1111.5728},
file = {:Users/idavidzon/Astro/all_papers/Santini et al. - 2012.pdf:pdf},
journal = {\aap},
keywords = {GSMF,galaxies: evolution,galaxies: fundamental parameters,galaxies: high-redshift,galaxies: luminosity function,high-z,mass function},
mendeley-tags = {GSMF,high-z},
month = {feb},
pages = {A33},
primaryClass = {astro-ph.CO},
title = {{The evolving slope of the stellar mass function at 0.6 {\le} z {\lt} 4.5 from deep WFC3 data}},
volume = {538},
year = {2012}
}

@article{Szalay99_chidetection,
author = {Szalay, Alexander S and Connolly, Andrew J and Szokoly, Gyula P},
journal = {\aj},
year = {1999},
volume = {117},
pages = {68},
local-url = {file://localhost/Users/hjmcc/Documents/Papers2/Articles/1999/Szalay/The%20Astronomical%20Journal%201999%20Szalay.pdf},
file = {{The Astronomical Journal 1999 Szalay.pdf:/Users/hjmcc/Documents/Papers2/Articles/1999/Szalay/The Astronomical Journal 1999 Szalay.pdf:application/pdf}},
}

@article{Bowler2015,
abstract = {We present a sample of 266 bright (-22.7 < M_UV < -20.5) Lyman-break galaxies at 5.5 < z < 6.5 found within a total of 1.65 square degrees of imaging in the UltraVISTA/COSMOS and UKIDSS UDS/SXDS fields. The deep near-infrared imaging available in the two independent fields, in addition to deep optical (including z'-band) data, enables the sample of z $\sim$ 6 star-forming galaxies to be securely detected long-ward of the break (in contrast to several previous studies). By simulating the potential contamination of our sample by cool galactic brown dwarfs, we find that the expected contamination rate of our initial sample is < 3 percent and that dwarf stars can be effectively removed by fitting dwarf star spectral templates to the photometry. At z $\sim$ 6 the galaxy surface density in the UltraVISTA field exceeds that in the UDS by a factor of $\sim$ 1.8, indicating strong cosmic variance even between degree-scale fields at z > 5. We calculate the bright end of the rest-frame Ultra-Violet (UV) luminosity function (LF) at z $\sim$ 6. The galaxy number counts are a factor of 2 lower than predicted by the recent LF determination by Bouwens et al.. In comparison to other smaller area studies, we find an evolution in the characteristic magnitude between z $\sim$ 5 and z $\sim$ 7 of dM* $\sim$ 0.4 mag, and show that a double power-law or a Schechter function can equally well describe the LF at z = 6. Furthermore, the bright-end of the LF appears to steepen from z $\sim$ 7 to z $\sim$ 5, which could indicate the onset of mass quenching or the rise of dust obscuration, a conclusion supported by comparing the observed LFs to a range of theoretical model predictions.},
author = {Bowler, R. A . A. and Dunlop, J. S. and McLure, R. J. and McCracken, H. J. and Furusawa, H. and Taniguchi, Y. and Fynbo, J. P. U. and Milvang-Jensen, B. and {Le Fevre}, O.},
file = {:Users/idavidzon/Astro/all_papers/Bowler et al. - 2015.pdf:pdf},
journal = {eprint arXiv:1411.2976},
keywords = {Astrophysics - Astrophysics of Galaxies,Astrophysics - Cosmology and Nongalactic Astrophys,LF,high-z},
mendeley-tags = {LF,high-z},
title = {{The galaxy luminosity function at z $\sim$ 6 and evidence for rapid evolution in the bright end from z $\sim$ 7 to 5}},
url = {http://adsabs.harvard.edu/abs/2014arXiv1411.2976B},
year = {2015}
}
@article{Capak2015,
abstract = {Evolution in the measured rest frame ultraviolet spectral slope and ultraviolet to optical flux ratios indicate a rapid evolution in the dust obscuration of galaxies during the first 3 billion years of cosmic time (z>4). This evolution implies a change in the average interstellar medium properties, but the measurements are systematically uncertain due to untested assumptions, and the inability to measure heavily obscured regions of the galaxies. Previous attempts to directly measure the interstellar medium in normal galaxies at these redshifts have failed for a number of reasons with one notable exception. Here we report measurements of the [CII] gas and dust emission in 9 typical ($\sim$1-4L*) star-forming galaxies $\sim$1 billon years after the big bang (z$\sim$5-6). We find these galaxies have >12x less thermal emission compared with similar systems $\sim$2 billion years later, and enhanced [CII] emission relative to the far-infrared continuum, confirming a strong evolution in the interstellar medium properties in the early universe. The gas is distributed over scales of 1-8 kpc, and shows diverse dynamics within the sample. These results are consistent with early galaxies having significantly less dust than typical galaxies seen at z<3 and being comparable to local low-metallicity systems.},
archivePrefix = {arXiv},
arxivId = {1503.07596},
author = {Capak, P. L. and Carilli, C. and Jones, G. and Casey, C. M. and Riechers, D. and Sheth, K. and Carollo, C. M. and Ilbert, O. and Karim, A. and LeFevre, O. and Lilly, S. and Scoville, N. and Smolcic, V. and Yan, L.},
eprint = {1503.07596},
journal = {\nat},
month = {mar},
pages = {22},
title = {{The Interstellar Medium In Galaxies Seen A Billion Years After The Big Bang}},
url = {http://arxiv.org/abs/1503.07596},
year = {2015}
}
@article{Stark2009,
abstract = {We present new measurements of the evolution in the Lyman break galaxy (LBG) population between z sime 4 and z sime 6. By utilizing the extensive multiwavelength data sets available in the GOODS fields, we identify 2443 B, 506 V, and 137 i'-band dropout galaxies likely to be at z ≈ 4, 5, and 6. For the subset of dropouts for which reliable Spitzer IRAC photometry is feasible (roughly 35% of the sample), we estimate luminosity-weighted ages and stellar masses. With the goal of understanding the duration of typical star formation episodes in galaxies at z gsim 4, we examine the distribution of stellar masses and ages as a function of cosmic time. We find that at a fixed rest-UV luminosity, the average stellar masses and ages of galaxies do not increase significantly between z sime 6 and 4. In order to maintain this near equilibrium in the average properties of high-redshift LBGs, we argue that there must be a steady flux of young, newly luminous objects at each successive redshift. When considered along with the short duty cycles inferred from clustering measurements, these results may suggest that galaxies are undergoing star formation episodes lasting only several hundred million years. In contrast to the unchanging relationship between the average stellar mass and rest-UV luminosity, we find that the number density of massive galaxies increases considerably with time over 4 lsim z lsim 6. Given this rapid increase of UV luminous massive galaxies, we explore the possibility that a significant fraction of massive (1011 M sun) z sime 2-3 distant red galaxies (DRGs) were in part assembled in an LBG phase at earlier times. Integrating the growth in the stellar mass function of actively forming LBGs over 4 lsim z lsim 6 down to z sime 2, we find that z gsim 3 LBGs could have contributed significantly to the quiescent DRG population, indicating that the intense star-forming systems probed by submillimeter observations are not the only route toward the assembly of DRGs at z sime 2.},
author = {Stark, Daniel P. and Ellis, Richard S. and Bunker, Andrew and Bundy, Kevin and Targett, Tom and Benson, Andrew and Lacy, Mark},
doi = {10.1088/0004-637X/697/2/1493},
file = {:Users/idavidzon/Astro/all_papers/Stark et al. - 2009.pdf:pdf},
issn = {0004-637X},
journal = {\apj},
keywords = {GSMF,LBG,galaxies: evolution,galaxies: formation,galaxies: high-redshift,galaxies: starburst,high-z,surveys,ultraviolet: galaxies},
mendeley-tags = {GSMF,LBG,high-z},
month = {jun},
number = {2},
pages = {1493--1511},
title = {{THE EVOLUTIONARY HISTORY OF LYMAN BREAK GALAXIES BETWEEN REDSHIFT 4 AND 6: OBSERVING SUCCESSIVE GENERATIONS OF MASSIVE GALAXIES IN FORMATION}},
url = {http://adsabs.harvard.edu/abs/2009ApJ...697.1493S},
volume = {697},
year = {2009}
}
@article{Graus2015,
abstract = {We constrain the evolution of the galaxy stellar mass function from 2 < z < 5 for galaxies with stellar masses as low as 10^5 Msun by combining star formation histories of Milky Way satellite galaxies derived from deep Hubble Space Telescope observations with merger trees from the ELVIS suite of N-body simulations. This approach extends our understanding more than two orders of magnitude lower in stellar mass than is currently possible by direct imaging. We find the faint end slopes of the mass functions to be alpha= -1.42(+0.07/-0.05) at z = 2 and alpha = -1.57^(+0.06/-0.06) at z = 5, and show the slope only weakly evolves from z = 5 to z = 0. Our findings are in stark contrast to a number of direct detection studies that suggest slopes as steep as alpha = -1.9 at these epochs. Such a steep slope would result in an order of magnitude too many luminous Milky Way satellites in a mass regime that is observationally complete (Mstar > 2*10^5 Msun at z = 0). The most recent studies from ZFOURGE and CANDELS also suggest flatter faint end slopes that are consistent with our results, but with a lower degree of precision. This work illustrates the strong connections between low and high-z observations when viewed through the lens of LCDM numerical simulations.},
archivePrefix = {arXiv},
arxivId = {1509.01250},
author = {Graus, Andrew S. and Bullock, James S. and Boylan-Kolchin, Michael and Weisz, Daniel R.},
eprint = {1509.01250},
keywords = {GSMF,high-z,low-mass,models},
mendeley-tags = {GSMF,high-z,low-mass,models},
month = {sep},
title = {{Push it to the limit: Local Group constraints on high-redshift stellar mass functions for Mstar > 10^5 Msun}},
url = {http://arxiv.org/abs/1509.01250},
year = {2015}
}
@article{Caputi2011,
abstract = {We have analysed a sample of 1292 4.5-mum-selected galaxies at z>= 3, over 0.6 deg2 of the UKIRT Infrared Deep Survey (UKIDSS) Ultra Deep Survey (UDS). Using photometry from the U band through 4.5 mum, we have obtained photometric redshifts and derived stellar masses for our sources. Only two of our galaxies potentially lie at z > 5. We have studied the galaxy stellar mass function at 3 <=z < 5, based on the 1213 galaxies in our catalogue with 4.5-mum magnitudes <=24.0. We find that (i) the number density of ? galaxies increased by a factor of >10 between z= 5 and 3, indicating that the assembly rate of these galaxies proceeded >20 times faster at these redshifts than at 0 < z < 2; (ii) the Schechter function slope alpha is significantly steeper than that displayed by the local stellar mass function, which is a consequence of both the steeper faint end and the absence of a pure exponential decline at the high-mass end; and (iii) the evolution of the comoving stellar mass density from z= 0 to 5 can be modelled as log10rhoM=-(0.05 ± 0.09)z2-(0.22 -/+ 0.32)z+ 8.69. At 3 <=z < 4, more than 30 per cent of the ? galaxies would be missed by optical surveys with R < 27 or z < 26. Thus, our study demonstrates the importance of deep mid-infrared surveys over large areas to perform a complete census of massive galaxies at high z and trace the early stages of massive galaxy assembly.},
author = {Caputi, K. I. and Cirasuolo, M. and Dunlop, J. S. and McLure, R. J. and Farrah, D. and Almaini, O.},
doi = {10.1111/j.1365-2966.2010.18118.x},
file = {:Users/idavidzon/Astro/all_papers/Caputi et al. - 2011.pdf:pdf},
issn = {00358711},
journal = {Monthly Notices of the Royal Astronomical Society},
keywords = {GSMF,galaxies: luminosity function,galaxies: statistics,high-z,infrared: galaxies,mass function},
mendeley-tags = {GSMF,high-z},
month = {may},
number = {1},
pages = {162--176},
title = {{The stellar mass function of the most-massive galaxies at 3 ≤z < 5 in the UKIDSS Ultra Deep Survey}},
url = {http://adsabs.harvard.edu/abs/2011MNRAS.413..162C},
volume = {413},
year = {2011}
}
@article{Bowler2012,
abstract = {We have exploited the new, deep, near-infrared UltraVISTA imaging of the Cosmological Evolution Survey (COSMOS) field, in tandem with deep optical and mid-infrared imaging, to conduct a new search for luminous galaxies at redshifts z $\sim$= 7. The year-one UltraVISTA data provide contiguous Y, J, H, Ks imaging over 1.5 deg2, reaching a 5sigma detection limit of Y + J $\sim$= 25 (AB mag, 2-arcsec-diameter aperture). The central $\sim$=1 deg2 of this imaging coincides with the final deep optical (u*, g, r, i) data provided by the Canada-France-Hawaii Telescope (CFHT) Legacy Survey and new deep Subaru/Suprime-Cam z'-band imaging obtained specifically to enable full exploitation of UltraVISTA. It also lies within the Hubble Space Telescope (HST) I814 band and Spitzer/Infrared Array Camera imaging obtained as part of the COSMOS survey. We have utilized this unique multiwavelength dataset to select galaxy candidates at redshifts z &gt; 6.5 by searching first for Y + J-detected objects which are undetected in the CFHT and HST optical data. This sample was then refined using a photometric redshift fitting code, enabling the rejection of lower redshift galaxy contaminants and cool galactic M, L, T dwarf stars. The final result of this process is a small sample of (at most) 10 credible galaxy candidates at z &gt; 6.5 (from over 200 000 galaxies detected in the year-one UltraVISTA data) which we present in this paper. The first four of these appear to be robust galaxies at z &gt; 6.5, and fitting to their stacked spectral energy distribution yields zphot = 6.98 ± 0.05 with a stellar mass M* $\sim$= 5 × 109 M&amp;sun; and rest-frame ultraviolet (UV) spectral slope beta $\sim$= -2.0 ± 0.2 (where flambda ∝ lambdabeta). The next three are also good candidates for z &gt; 6.5 galaxies, but the possibility that they are dwarf stars cannot be completely excluded. Our final subset of three additional candidates is afflicted not only by potential dwarf star contamination, but also contains objects likely to lie at redshifts just below z = 6.5. We show that the three even-brighter z ≳ 7 galaxy candidates reported in the COSMOS field by Capak et al. are in fact all lower redshift galaxies at z $\sim$= 1.5-3.5. Consequently the new z $\sim$= 7 galaxies reported here are the first credible z $\sim$= 7 Lyman-break galaxies discovered in the COSMOS field and, as the most UV luminous discovered to date at these redshifts, are prime targets for deep follow-up spectroscopy. We explore their physical properties, and briefly consider the implications of their inferred number density for the form of the galaxy luminosity function at z $\sim$= 7.},
author = {Bowler, R. A. A. and Dunlop, J. S. and McLure, R. J. and McCracken, H. J. and Milvang-Jensen, B. and Furusawa, H. and Fynbo, J. P. U. and {Le F{\`{e}}vre}, O. and Holt, J. and Ideue, Y. and Ihara, Y. and Rogers, A. B. and Taniguchi, Y.},
doi = {10.1111/j.1365-2966.2012.21904.x},
issn = {00358711},
journal = {Monthly Notices of the Royal Astronomical Society},
keywords = {galaxies: evolution,galaxies: formation,galaxies: high-redshift,high-z,photoz},
mendeley-tags = {high-z,photoz},
month = {nov},
number = {4},
pages = {2772--2788},
title = {{Discovery of bright z ≃ 7 galaxies in the UltraVISTA survey}},
url = {http://adsabs.harvard.edu/abs/2012MNRAS.426.2772B},
volume = {426},
year = {2012}
}
@article{Nickel2015,
abstract = {Relational machine learning studies methods for the statistical analysis of relational, or graph-structured, data. In this paper, we provide a review of how such statistical models can be "trained" on large knowledge graphs, and then used to predict new facts about the world (which is equivalent to predicting new edges in the graph). In particular, we discuss two different kinds of statistical relational models, both of which can scale to massive datasets. The first is based on tensor factorization methods and related latent variable models. The second is based on mining observable patterns in the graph. We also show how to combine these latent and observable models to get improved modeling power at decreased computational cost. Finally, we discuss how such statistical models of graphs can be combined with text-based information extraction methods for automatically constructing knowledge graphs from the Web. In particular, we discuss Google's Knowledge Vault project.},
annote = {bho},
archivePrefix = {arXiv},
arxivId = {1503.0759},
author = {Nickel, Maximilian and Murphy, Kevin and Tresp, Volker and Gabrilovich, Evgeniy},
eprint = {1503.0759},
keywords = {Astrophysics - Astrophysics of Galaxies},
language = {en},
month = {mar},
title = {{A Review of Relational Machine Learning for Knowledge Graphs: From Multi-Relational Link Prediction to Automated Knowledge Graph Construction}},
url = {http://adsabs.harvard.edu/abs/2015arXiv150307596C},
year = {2015}
}
@article{Caputi2015,
abstract = {We have analysed a sample of 574 Spitzer 4.5 micron-selected galaxies with [4.5]<23 and Ks>24 (AB) over the UltraVISTA ultra-deep COSMOS field. Our aim is to investigate whether these mid-IR bright, near-IR faint sources contribute significantly to the overall population of massive galaxies at redshifts z>=3. By performing a spectral energy distribution (SED) analysis using up to 30 photometric bands, we have determined that the redshift distribution of our sample peaks at redshifts z$\sim$2.5-3.0, and $\sim$32% of the galaxies lie at z>=3. We have studied the contribution of these sources to the galaxy stellar mass function (GSMF) at high redshifts. We found that the [4.5]<23, Ks>24 galaxies produce a negligible change to the GSMF previously determined for Ks<24 sources at 3=<z<4, but their contribution is more important at 4=<z<5, accounting for >$\sim$50% of the galaxies with stellar masses Mst>$\sim$6 x 10^10 Msun. We also constrained the GSMF at the highest-mass end (Mst>$\sim$2 x 10^11 Msun) at z>=5. From their presence at 5=<z<6, and virtual absence at higher redshifts, we can pinpoint quite precisely the moment of appearance of the first most massive galaxies as taking place in the $\sim$0.2 Gyr of elapsed time between z$\sim$6 and z$\sim$5. Alternatively, if very massive galaxies existed earlier in cosmic time, they should have been significantly dust-obscured to lie beyond the detection limits of current, large-area, deep near-IR surveys.},
archivePrefix = {arXiv},
arxivId = {1505.05721},
author = {Caputi, K. I. and Ilbert, O. and Laigle, C. and McCracken, H. J. and Fevre, O. Le and Fynbo, J. and Milvang-Jensen, B. and Capak, P. and Salvato, M. and Taniguchi, Y.},
eprint = {1505.05721},
file = {:Users/idavidzon/Astro/all_papers/Caputi et al. - 2015.pdf:pdf},
keywords = {GSMF,high-z},
mendeley-tags = {GSMF,high-z},
month = {may},
pages = {16},
title = {{Spitzer bright, UltraVISTA faint sources in COSMOS: the contribution to the overall population of massive galaxies at z=3-7}},
url = {http://arxiv.org/abs/1505.05721},
year = {2015}
}
@article{Smit2012,
abstract = {We combine recent estimates of dust extinction at z $\sim$ 4-7 with UV luminosity function (LF) determinations to derive star formation rate (SFR) functions at z $\sim$ 4-7. SFR functions provide a more physical description of galaxy buildup at high redshift and allow for direct comparisons to SFRs at lower redshifts determined by a variety of techniques. Our SFR functions are derived from well-established z $\sim$ 4-7 UV LFs, UV-continuum slope trends with redshift and luminosity, and infrared excess (IRX)-beta relations. They are well described by Schechter relations. We extend the comparison baseline for SFR functions to z $\sim$ 2 by considering recent determinations of the Halpha and mid-IR LFs. The low-end slopes of the SFR functions are flatter than for the UV LFs, Deltaalpha $\sim$ +0.13, and show no clear evolution with cosmic time (z $\sim$ 0-7). In addition, we find that the characteristic value SFR* from the Schechter fit to the SFR function exhibits consistent, and substantial, linear growth as a function of redshift from $\sim$5 M &amp;sun; yr-1 at z $\sim$ 8, 650 Myr after the big bang, to $\sim$100 M &amp;sun; yr-1 at z $\sim$ 2, $\sim$2.5 Gyr later. Recent results at z $\sim$ 10, close to the onset of galaxy formation, are consistent with this trend. The uniformity of this evolution is even greater than seen in the UV LF over the redshift range z $\sim$ 2-8, providing validation for our dust corrections. These results provide strong evidence that galaxies build up uniformly over the first 3 Gyr of cosmic time.},
archivePrefix = {arXiv},
arxivId = {astro-ph.CO/1204.3626},
author = {Smit, Renske and Bouwens, Rychard J. and Franx, Marijn and Illingworth, Garth D. and Labb{\'{e}}, Ivo and Oesch, Pascal a. and van Dokkum, Pieter G.},
doi = {10.1088/0004-637X/756/1/14},
eprint = {1204.3626},
file = {:Users/idavidzon/Astro/all_papers/Smit et al. - 2012.pdf:pdf},
issn = {0004-637X},
journal = {\apj},
keywords = {color figures,evolution,galaxies,high-redshift,online-only material},
number = {1},
pages = {14},
primaryClass = {astro-ph.CO},
title = {{THE STAR FORMATION RATE FUNCTION FOR REDSHIFT z ∼ 4-7 GALAXIES: EVIDENCE FOR A UNIFORM BUILDUP OF STAR-FORMING GALAXIES DURING THE FIRST 3 Gyr OF COSMIC TIME}},
volume = {756},
year = {2012}
}
@article{Duncan2014,
abstract = {We measure new estimates for the galaxy stellar mass function and star formation rates for samples of galaxies at z ˜ 4, 5, 6 and 7 using data in the CANDELS GOODS South field. The deep near-infrared observations allow us to construct the stellar mass function at z &gt;= 6 directly for the first time. We estimate stellar masses for our sample by fitting the observed spectral energy distributions with synthetic stellar populations, including nebular line and continuum emission. The observed UV luminosity functions for the samples are consistent with previous observations; however, we find that the observed MUV-M* relation has a shallow slope more consistent with a constant mass-to-light ratio and a normalization which evolves with redshift. Our stellar mass functions have steep low-mass slopes (alpha ≈ -1.9), steeper than previously observed at these redshifts and closer to that of the UV luminosity function. Integrating our new mass functions, we find the observed stellar mass density evolves from log _{10} rho _{*} = 6.64^{+0.58}_{-0.89} at z ˜ 7 to 7.36 ± 0.06 M&amp;sun; Mpc- 3 at z ˜ 4. Finally, combining the measured UV continuum slopes (beta) with their rest-frame UV luminosities, we calculate dust-corrected star formation rates (SFR) for our sample. We find the specific SFR for a fixed stellar mass increases with redshift whilst the global SFR density falls rapidly over this period. Our new SFR density estimates are higher than previously observed at this redshift.},
author = {Duncan, K. and Conselice, C. J. and Mortlock, A. and Hartley, W. G. and Guo, Y. and Ferguson, H. C. and Dave, R. and Lu, Y. and Ownsworth, J. and Ashby, M. L. N. and Dekel, A. and Dickinson, M. and Faber, S. and Giavalisco, M. and Grogin, N. and Kocevski, D. and Koekemoer, A. and Somerville, R. S. and White, C. E.},
doi = {10.1093/mnras/stu1622},
file = {:Users/idavidzon/Astro/all_papers/Duncan et al. - 2014.pdf:pdf},
issn = {0035-8711},
journal = {\mnras},
keywords = {GSMF,galaxies: evolution,galaxies: formation,galaxies: high-redshift,galaxies: luminosity function,mass function},
mendeley-tags = {GSMF},
month = {sep},
number = {3},
pages = {2960--2984},
title = {{The mass evolution of the first galaxies: stellar mass functions and star formation rates at 4 < z < 7 in the CANDELS GOODS-South field}},
url = {http://adsabs.harvard.edu/abs/2014MNRAS.444.2960D},
volume = {444},
year = {2014}
}
@article{Wilkins2013a,
abstract = {By combining optical and near-IR observations from the Hubble Space Telescope with near-IR photometry from the Spitzer Space Telescope, it is possible to measure the rest-frame UV-optical colours of galaxies at z = 4-8. The UV-optical spectral energy distribution of star formation dominated galaxies is the result of several different factors. These include the joint distribution of stellar masses, ages and metallicities (solely responsible for the pure stellar spectral energy distribution), and the subsequent reprocessing by dust and gas in the interstellar medium. Using a large cosmological hydrodynamical simulation (MassiveBlack-II), we investigate the predicted spectral energy distributions of galaxies at high redshift with a particular emphasis on assessing the potential contribution of nebular emission. We find that the average (median) pure stellar UV-optical colour correlates with both luminosity and redshift such that galaxies at lower redshift and higher luminosity are typically redder. Assuming that the escape fraction of ionizing photons is close to zero, the effect of nebular emission is to redden the UV-optical 1500 - Vw colour by, on average, 0.4 mag at z = 8 declining to 0.25 mag at z = 4. Young and low-metallicity stellar populations, which typically have bluer pure stellar UV-optical colours, produce larger ionizing luminosities and are thus more strongly affected by the reddening effects of nebular emission. This causes the distribution of 1500 - Vw colours to narrow and the trends with luminosity and redshift to weaken. The strong effect of nebular emission leaves observed-frame colours critically sensitive to the redshift of the source. For example, increasing the redshift by 0.1 can result in observed-frame colours changing by up to ˜0.6. These predictions reinforce the need to include nebular emission when modelling the spectral energy distributions of galaxies at high redshift and also highlight the difficultly in interpreting the observed colours of individual galaxies without precise redshift information.},
annote = {nebular emission line reference},
author = {Wilkins, S. M. and Coulton, W. and Caruana, J. and Croft, R. and Matteo, T. D. and Khandai, N. and Feng, Y. and Bunker, A. and Elbert, H.},
doi = {10.1093/mnras/stt1471},
issn = {0035-8711},
journal = {Monthly Notices of the Royal Astronomical Society},
keywords = {SED fitting,galaxies: high-redshift,galaxies: photometry,high-z,methods},
mendeley-tags = {SED fitting,high-z,methods},
month = {sep},
number = {4},
pages = {2885--2895},
title = {{Theoretical predictions for the effect of nebular emission on the broad-band photometry of high-redshift galaxies}},
url = {http://adsabs.harvard.edu/abs/2013MNRAS.435.2885W},
volume = {435},
year = {2013}
}
@article{Wilkins2008,
abstract = {We present a compilation of measurements of the stellar mass density as a function of redshift. Using this stellar mass history we obtain a star formation history and compare it to the instantaneous star formation history. For z < 0.7 there is good agreement between the two star formation histories. At higher redshifts the instantaneous indicators suggest star formation rates larger than that implied by the evolution of the stellar mass density. This discrepancy peaks at z = 3 where instantaneous indicators suggest a star formation rate around 0.6 dex higher than those of the best fit to the stellar mass history. We discuss a variety of explanations for this inconsistency, such as inaccurate dust extinction corrections, incorrect measurements of stellar masses and a possible evolution of the stellar initial mass function.},
author = {Wilkins, Stephen M. and Trentham, Neil and Hopkins, Andrew M.},
doi = {10.1111/j.1365-2966.2008.12885.x},
file = {:Users/idavidzon/Astro/all_papers/Wilkins, Trentham, Hopkins - 2008.pdf:pdf},
issn = {0035-8711},
journal = {\mnras},
keywords = {SFRD,SMD,cosmology: observations,galaxies: stellar content},
mendeley-tags = {SFRD,SMD},
month = {apr},
number = {2},
pages = {687--694},
title = {{The evolution of stellar mass and the implied star formation history}},
url = {http://adsabs.harvard.edu/abs/2008MNRAS.385..687W},
volume = {385},
year = {2008}
}
@article{Clements2015,
abstract = {We show that the use of red colour as the basis for selecting candidate high redshift dusty galaxies from surveys made with Herschel has proved highly successful. The highest redshift such object, HFLS3, lies at z=6.34 and numerous other sources have been found. Spectroscopic followup confirms that most of these lie at z>4. These sources are found in such numbers that they represent a challenge to current models of galaxy evolution. We also examine the prospects for finding dusty galaxies at still higher redshifts. These would not appear in the SPIRE surveys from Herschel but would be detected in longer wavelength, submm, surveys. Several such `SPIRE-dropouts' have been found and are now subject to followup observations.},
annote = {Dusty galaxies at z&gt;4},
archivePrefix = {arXiv},
arxivId = {1511.03060},
author = {Clements, David L and Greenslade, Josh and Riechers, Dominik A. and Wardlow, Julie and Perez-Fournon, Ismael and Collective, The HerMES Red and HerMES, The and Consortia, H-ATLAS},
eprint = {1511.03060},
file = {::},
keywords = {dust,high-z},
mendeley-tags = {dust,high-z},
month = {nov},
pages = {4},
title = {{Dusty Galaxies at the Highest Redshifts}},
url = {http://arxiv.org/abs/1511.03060},
year = {2015}
}
@article{Lanzetta1996,
abstract = {Analysis of the deepest available images of the sky, obtained by the Hubble Space Telescope, reveals a large number of candidate high-redshift galaxies. A catalogue of 1,683 objects is presented, with estimated redshifts ranging from z = 0 to z &gt; 6. The high-redshift objects are interpreted as regions of star formation associated with the progenitors of present-day normal galaxies, at epochs that may reach back 95% of the time to the Big Bang.},
author = {Lanzetta, Kenneth M. and Yahil, Amos and Fern{\'{a}}ndez-Soto, Alberto},
doi = {10.1038/381759a0},
issn = {0028-0836},
journal = {\nat},
month = {jun},
number = {6585},
pages = {759--763},
title = {{Star-forming galaxies at very high redshifts}},
url = {http://adsabs.harvard.edu/abs/1996Natur.381..759L},
volume = {381},
year = {1996}
}
@article{Huang2015,
abstract = {We study the stellar population properties of the IRAC-detected $6 \lesssim z \lesssim 10$ galaxy candidates from the Spitzer UltRa Faint SUrvey Program (SURFS UP). Using the Lyman Break selection technique, we find a total of 16 new galaxy candidates at $6 \lesssim z \lesssim 10$ with $S/N \geq 3$ in at least one of the IRAC $3.6\mu$m and $4.5\mu$m bands. According to the best mass models available for the surveyed galaxy clusters, these IRAC-detected galaxy candidates are magnified by factors of $\sim 1.2$--$5.5$. We find that the IRAC-detected $6 \lesssim z \lesssim 10$ sample is likely not a homogeneous galaxy population: some are relatively massive (stellar mass as high as $4 \times 10^9\,M_{\odot}$) and evolved (age $\lesssim 500$ Myr) galaxies, while others are less massive ($M_{\text{stellar}}\sim 10^8\,M_{\odot}$) and very young ($\sim 10$ Myr) galaxies with strong nebular emission lines that boost their rest-frame optical fluxes. We identify two Ly$\alpha$ emitters in our sample from the Keck DEIMOS spectra, one at $z_{\text{Ly}\alpha}=6.76$ (in RXJ1347) and one at $z_{\text{Ly}\alpha}=6.32$ (in MACS0454). We show that IRAC $[3.6]-[4.5]$ color, when combined with photometric redshift, can be used to identify galaxies likely with strong nebular emission lines within certain redshift windows.},
annote = {use of IRAC colours},
archivePrefix = {arXiv},
arxivId = {1504.02099},
author = {Huang, Kuang-Han and Brada{\v{c}}, Maru{\v{s}}a and Lemaux, Brian C. and Ryan,, R. E. and Hoag, Austin and Castellano, Marco and Amor{\'{I}}n, Ricardo and Fontana, Adriano and Brammer, Gabriel B. and Cain, Benjamin and Lubin, L. M. and Merlin, Emiliano and Schmidt, Kasper B. and Schrabback, Tim and Treu, Tommaso and Gonzalez, Anthony H. and {Von Der Linden}, Anja and Knight, Robert I.},
eprint = {1504.02099},
keywords = {LBG},
mendeley-tags = {LBG},
month = {apr},
title = {{Spitzer UltRa Faint SUrvey Program (SURFS UP). II. IRAC-Detected Lyman-Break Galaxies at 6 < z < 10 Behind Strong-Lensing Clusters}},
url = {http://arxiv.org/abs/1504.02099},
year = {2015}
}
@article{Scott2015,
abstract = {We present high-redshift predictions of the star-formation-rate distribution function (SFR DF), UV luminosity function (UV LF), galactic stellar mass function (GSMF), and specific star-formation rates (sSFRs) of galaxies from the latest version of the Munich semi-analytic model L-Galaxies. We find a good fit to both the shape and normalisation of the SFR DF at $z=4-7$, apart from a slight under-prediction at the low SFR end at $z=4$. Likewise, we find a good fit to the faint number counts for the observed UV LF; at brighter magnitudes our predictions lie below the observations, increasingly so at higher redshifts. At all redshifts and magnitudes, the raw (unattenuated) number counts for the UV LF lie above the observations. Because of the good agreement with the SFR we interpret our under-prediction as an over-estimate of the amount of dust in the model for the brightest galaxies, especially at high-redshift. While the shape of our GSMF matches that of the observations, we lie between (conflicting) observations at $z=4-5$, and under-predict at $z=6-7$. The sSFRs of our model galaxies show the observed trend of increasing normalisation with redshift, but do not reproduce the observed mass dependence. Overall, we conclude that the latest version of L-Galaxies, which is tuned to match observations at $z\leq3$, does a fair job of reproducing the observed properties of galaxies at $z\geq4$. More work needs to be done on understanding observational bias at high-redshift, and upon the dust model, before strong conclusions can be drawn on how to interpret remaining discrepancies between the model and observations.},
archivePrefix = {arXiv},
arxivId = {1504.03321},
author = {Clay, Scott and Thomas, Peter and Wilkins, Stephen and Henriques, Bruno},
doi = {10.1093/mnras/stv818},
eprint = {1504.03321},
file = {:Users/idavidzon/Astro/all_papers/Clay et al. - 2015.pdf:pdf},
journal = {ArXiv e-prints},
keywords = {GSMF,high-z,sims},
mendeley-tags = {GSMF,high-z,sims},
month = {apr},
pages = {12},
title = {{Galaxy formation in the PLANCK cosmology IV: the high-redshift universe}},
url = {http://arxiv.org/abs/1504.03321},
year = {2015}
}
@article{Wilkins2013,
abstract = {We investigate the evolution of the galaxy stellar mass function at high redshift (z >= 5) using a pair of large cosmological hydrodynamical simulations: MassiveBlack and MassiveBlack-II. By combining these simulations, we can study the properties of galaxies with stellar masses greater than 108 M&sun; h-1 and (comoving) number densities of log10(phi [Mpc-3 dex-1 h3]) > -8. Observational determinations of the galaxy stellar mass function at very high redshift typically assume a relation between the observed ultraviolet (UV) luminosity and stellar mass-to-light ratio which is applied to high-redshift samples in order to estimate stellar masses. This relation can also be measured from the simulations. We do this, finding two significant differences with the usual observational assumption: it evolves strongly with redshift and has a different shape. Using this relation to make a consistent comparison between galaxy stellar mass functions, we find that at z = 6 and above the simulation predictions are in good agreement with observed data over the whole mass range. Without using the correct UV luminosity and stellar mass-to-light ratio, the discrepancy would be up to two orders of magnitude for large galaxies (>1010 M&sun; h-1). At z = 5, however, the stellar mass function for low-mass galaxies (<109 M&sun; h-1) is overpredicted by factors of a few, consistent with the behaviour of the UV luminosity function, and perhaps a sign that feedback in the simulation is not efficient enough for these galaxies.},
annote = {Mah, il confronto con la Mf di Gonzalez non va benissimo. Peccato che non si possa usare come dimostrazione dei limiti del metodo L_UV--&gt;MF},
author = {Wilkins, S. M. and Matteo, T. D. and Croft, R. and Khandai, N. and Feng, Y. and Bunker, A. and Coulton, W.},
doi = {10.1093/mnras/sts480},
file = {:Users/idavidzon/Astro/all_papers/Wilkins et al. - 2013.pdf:pdf},
issn = {0035-8711},
journal = {\mnras},
keywords = {galaxies: high-redshift,galaxies: luminosity function,galaxies: stellar content,high-z,mass function,sims},
mendeley-tags = {high-z,sims},
month = {jan},
number = {3},
pages = {2098--2103},
title = {{Confronting predictions of the galaxy stellar mass function with observations at high redshift}},
url = {http://adsabs.harvard.edu/abs/2013MNRAS.429.2098W},
volume = {429},
year = {2013}
}
@article{Duncan2015,
abstract = {We present a new analysis of the ionizing emissivity ($\dot{N}_{\rm{ion}}$, s$^{-1}$ Mpc$^{-3}$) for galaxies during the epoch of reionization and their potential for completing and maintaining reionization. We use extensive SED modelling -- incorporating two plausible mechanisms for the escape of Lyman continuum photon -- to explore the range and evolution of ionizing efficiencies consistent with new results on galaxy colours ($\beta$) during this epoch. We estimate $\dot{N}_{\rm{ion}}$ for the latest observations of the luminosity and star-formation rate density at $z<10$, outlining the range of emissivity histories consistent with our new model. Given the growing observational evidence for a UV colour-magnitude relation in high-redshift galaxies, we find that for any plausible evolution in galaxy properties, red (brighter) galaxies are less efficient at producing ionizing photons than their blue (fainter) counterparts. The assumption of a redshift and luminosity evolution in $\beta$ leads to two important conclusions. Firstly, the ionizing efficiency of galaxies naturally increases with redshift. Secondly, for a luminosity dependent ionizing efficiency, we find that galaxies down to a rest-frame magnitude of $M_{\rm{UV}} \approx -15$ alone can potentially produce sufficient numbers of ionizing photons to maintain reionization as early as $z\sim8$ for a clumping factor of $C_{\rm{H {\small II}}} \leq 3$.},
archivePrefix = {arXiv},
arxivId = {1505.01846},
author = {Duncan, Kenneth and Conselice, Christopher J},
eprint = {1505.01846},
file = {:Users/idavidzon/Astro/all_papers/Duncan, Conselice - 2015.pdf:pdf},
keywords = {SED,high-z,inization},
mendeley-tags = {SED,high-z,inization},
month = {may},
title = {{Powering reionization: assessing the galaxy ionizing photon budget at $z < 10$}},
url = {http://arxiv.org/abs/1505.01846},
year = {2015}
}
@article{Reddy2015,
abstract = {We present results on the dust attenuation curve of z$\sim$2 galaxies using early observations from the MOSFIRE Deep Evolution Field (MOSDEF) survey. Our sample consists of 224 star-forming galaxies with nebular spectroscopic redshifts in the range z= 1.36-2.59 and high S/N measurements of, or upper limits on, the H-alpha and H-beta emission lines obtained with Keck/MOSFIRE. We construct composite SEDs of galaxies in bins of specific SFR and Balmer optical depth in order to directly constrain the dust attenuation curve from the UV through near-IR for typical star-forming galaxies at high redshift. Our results imply an attenuation curve that is very similar to the SMC extinction curve at wavelengths redward of 2500 Angstroms. At shorter wavelengths, the shape of the curve is identical to that of the Calzetti relation, but with a lower normalization (R_V). Hence, the new attenuation curve results in SFRs that are $\sim$20% lower, and log stellar masses that are 0.16 dex lower, than those obtained with the Calzetti attenuation curve. Moreover, we find that the difference in the reddening---and the total attenuation---of the ionized gas and stellar continuum correlates strongly with SFR, such that for dust-corrected SFRs larger than 20 Msun/yr assuming a Chabrier IMF, the nebular emission lines suffer an increasing degree of obscuration relative to the continuum. A simple model that can account for these trends is one in which the UV through optical stellar continuum is dominated by a population of less reddened stars, while the nebular line and bolometric luminosities become increasingly dominated by dustier stellar populations for galaxies with large SFRs, as a result of the increased dust enrichment that accompanies such galaxies. Consequently, UV- and SED-based SFRs may underestimate the total SFR at even modest levels of $\sim$20 Msun/yr. [Abridged]},
annote = {They propose a new attenuation curve.
Lower norm. than Calzetti's},
archivePrefix = {arXiv},
arxivId = {1504.02782},
author = {Reddy, Naveen A. and Kriek, Mariska and Shapley, Alice E. and Freeman, William R. and Siana, Brian and Coil, Alison L. and Mobasher, Bahram and Price, Sedona H. and Sanders, Ryan L. and Shivaei, Irene},
eprint = {1504.02782},
file = {:Users/idavidzon/Astro/all_papers/Reddy et al. - 2015.pdf:pdf},
journal = {\apj},
keywords = {dust,extinction curve},
mendeley-tags = {dust,extinction curve},
month = {apr},
pages = {24},
title = {{The MOSDEF Survey: Measurements of Balmer Decrements and the Dust Attenuation Curve at Redshifts z$\sim$1.4-2.6}},
url = {http://arxiv.org/abs/1504.02782},
year = {2015}
}
@article{Ashby2015,
abstract = {The Spitzer-Cosmic Assembly Deep Near-Infrared Extragalactic Legacy Survey (S-CANDELS; PI G. Fazio) is a Cycle 8 Exploration Program designed to detect galaxies at very high redshifts (z > 5). To mitigate the effects of cosmic variance and also to take advantage of deep coextensive coverage in multiple bands by the Hubble Space Telescope Multi-Cycle Treasury Program CANDELS, S-CANDELS was carried out within five widely separated extragalactic fields: the UKIDSS Ultra-Deep Survey, the Extended Chandra Deep Field South, COSMOS, the HST Deep Field North, and the Extended Groth Strip. S-CANDELS builds upon the existing coverage of these fields from the Spitzer Extended Deep Survey (SEDS) by increasing the integration time from 12 hours to a total of 50 hours but within a smaller area, 0.16 square degrees. The additional depth significantly increases the survey completeness at faint magnitudes. This paper describes the S-CANDELS survey design, processing, and publicly-available data products. We present IRAC dual-band 3.6+4.5 micron catalogs reaching to a depth of 26.5 AB mag. Deep IRAC counts for the roughly 135,000 galaxies detected by S-CANDELS are consistent with models based on known galaxy populations. The increase in depth beyond earlier Spitzer/IRAC surveys does not reveal a significant additional contribution from discrete sources to the diffuse Cosmic Infrared Background (CIB). Thus it remains true that only roughly half of the estimated CIB flux from COBE/DIRBE is resolved.},
archivePrefix = {arXiv},
arxivId = {1506.01323},
author = {Ashby, M. L. N. and Willner, S. P. and Fazio, G. G. and Dunlop, J. S. and Egami, E. and Faber, S. M. and Ferguson, H. C. and Grogin, N. A. and Hora, J. L. and Huang, J. -S. and Koekemoer, A. M. and Labbe, I. and Wang, Z.},
eprint = {1506.01323},
file = {:Users/idavidzon/Astro/all_papers/Ashby et al. - 2015.pdf:pdf},
keywords = {high-z,survey},
mendeley-tags = {high-z,survey},
month = {jun},
pages = {23},
title = {{S-CANDELS: The Spitzer-Cosmic Assembly Near-Infrared Deep Extragalactic Survey. Survey Design, Photometry, and Deep IRAC Source Counts}},
url = {http://arxiv.org/abs/1506.01323},
year = {2015}
}


@article{scoville_cosmic_2007,
	title = {The {Cosmic} {Evolution} {Survey} ({COSMOS}): {Overview}},
	volume = {172},
	issn = {0067-0049},
	shorttitle = {The {Cosmic} {Evolution} {Survey} ({COSMOS})},
	url = {https://ui.adsabs.harvard.edu/abs/2007ApJS..172....1S/abstract},
	doi = {10.1086/516585},
	abstract = {The Cosmic Evolution Survey (COSMOS) is designed to probe the correlated evolution of galaxies, star formation, active galactic nuclei (AGNs), and dark matter (DM) with large-scale structure (LSS) over the redshift range z\&gt;0.5-6. The survey includes multiwavelength imaging and spectroscopy from X-ray-to-radio wavelengths covering a 2 deg{\textless}SUP{\textgreater}2{\textless}/SUP{\textgreater} area, including HST imaging. Given the very high sensitivity and resolution of these data sets, COSMOS also provides unprecedented samples of objects at high redshift with greatly reduced cosmic variance, compared to earlier surveys. Here we provide a brief overview of the survey strategy, the characteristics of the major COSMOS data sets, and a summary the science goals. {\textless}P /{\textgreater}Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555 also based on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan; the XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA; the European Southern Observatory under Large Program 175.A-0839, Chile; Kitt Peak National Observatory, Cerro Tololo Inter-American Observatory, and the National Optical Astronomy Observatory, which are operated by the AURA, Inc., under cooperative agreement with the National Science Foundation; the National Radio Astronomy Observatory, which is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.; and the Canada-France-Hawaii Telescope with MegaPrime/MegaCam operated as a joint project by the CFHT Corporation, CEA/DAPNIA, the NRC and CADC of Canada, the CNRS of France, TERAPIX, and the University of Hawaii.},
	language = {en},
	number = {1},
	urldate = {2019-11-17},
	journal = {ApJS},
	author = {Scoville, N. and Aussel, H. and Brusa, M. and Capak, P. and Carollo, C. M. and Elvis, M. and Giavalisco, M. and Guzzo, L. and Hasinger, G. and Impey, C. and Kneib, J.-P. and LeFevre, O. and Lilly, S. J. and Mobasher, B. and Renzini, A. and Rich, R. M. and Sanders, D. B. and Schinnerer, E. and Schminovich, D. and Shopbell, P. and Taniguchi, Y. and Tyson, N. D.},
	month = sep,
	year = {2007},
	pages = {1}
}

@article{laigle_cosmos2015_2016,
	title = {The {COSMOS}2015 {Catalog}: {Exploring} the 1 {\textless} z {\textless} 6 {Universe} with {Half} a {Million} {Galaxies}},
	volume = {224},
	issn = {0067-0049},
	shorttitle = {The {COSMOS}2015 {Catalog}},
	url = {http://adsabs.harvard.edu/abs/2016ApJS..224...24L},
	doi = {10.3847/0067-0049/224/2/24},
	abstract = {We present the COSMOS201524 catalog, which contains precise 
photometric redshifts and stellar masses for more than half a million
objects over the 2deg2 COSMOS field. Including new
\{\{YJHK\}\}\{\{s\}\} images from the UltraVISTA-DR2 survey, Y-band
images from Subaru/Hyper-Suprime-Cam, and infrared data from the Spitzer
Large Area Survey with the Hyper-Suprime-Cam Spitzer legacy program,
this near-infrared-selected catalog is highly optimized for the study of
galaxy evolution and environments in the early universe. To maximize
catalog completeness for bluer objects and at higher redshifts, objects
have been detected on a χ 2 sum of the
\{\{YJHK\}\}\{\{s\}\} and z ++ images. The catalog
contains ˜ 6× \{10\}5 objects in the 1.5
deg2 UltraVISTA-DR2 region and ˜ 1.5×
\{10\}5 objects are detected in the “ultra-deep
stripes” (0.62 deg2) at \{K\}\{\{s\}\}≤slant
24.7 (3σ, 3″, AB magnitude). Through a comparison with the
zCOSMOS-bright spectroscopic redshifts, we measure a photometric
redshift precision of \{σ \}\{\vphantom{\}}\{\vphantom{\}}Δ
\vphantom{\{}\}z/(1+\{z\vphantom{\{}\}s)\} = 0.007 and a catastrophic failure
fraction of η = 0.5\%. At 3{\textbackslash}lt z{\textbackslash}lt 6, using the unique database of
spectroscopic redshifts in COSMOS, we find \{σ \}\{\vphantom{\}}\{\vphantom{\}}Δ
\vphantom{\{}\}z/(1+\{z\vphantom{\{}\}s)\} = 0.021 and η = 13.2 \% . The deepest
regions reach a 90\% completeness limit of
\{10\}10\{M\}⊙ to z = 4. Detailed comparisons of
the color distributions, number counts, and clustering show excellent
agreement with the literature in the same mass ranges. COSMOS2015
represents a unique, publicly available, valuable resource with which to
investigate the evolution of galaxies within their environment back to
the earliest stages of the history of the universe. The COSMOS2015
catalog is distributed via anonymous ftp and through the usual
astronomical archive systems (CDS, ESO Phase 3, IRSA).},
	urldate = {2018-09-29},
	journal = {ApJS},
	author = {Laigle, C. and McCracken, H. J. and Ilbert, O. and Hsieh, B. C. and Davidzon, I. and Capak, P. and Hasinger, G. and Silverman, J. D. and Pichon, C. and Coupon, J. and Aussel, H. and Le Borgne, D. and Caputi, K. and Cassata, P. and Chang, Y.-Y. and Civano, F. and Dunlop, J. and Fynbo, J. and Kartaltepe, J. S. and Koekemoer, A. and Le Fèvre, O. and Le Floc'h, E. and Leauthaud, A. and Lilly, S. and Lin, L. and Marchesi, S. and Milvang-Jensen, B. and Salvato, M. and Sanders, D. B. and Scoville, N. and Smolcic, V. and Stockmann, M. and Taniguchi, Y. and Tasca, L. and Toft, S. and Vaccari, Mattia and Zabl, J.},
	month = jun,
	year = {2016},
	keywords = {galaxies: high-redshift, galaxies: photometry, catalogs, galaxies: evolution, methods: observational, techniques: photometric},
	pages = {24}
}

@article{moutard_vipers_2016,
	title = {The {VIPERS} {Multi}-{Lambda} {Survey}. {I}. {UV} and near-{IR} observations, multi-colour catalogues, and photometric redshifts},
	volume = {590},
	issn = {0004-6361},
	url = {http://adsabs.harvard.edu/abs/2016A%26A...590A.102M},
	doi = {10.1051/0004-6361/201527945},
	abstract = {We present observations collected in the CFHTLS-VIPERS region in the 
ultraviolet with the GALEX satellite (far- and near-ultraviolet
channels) and in the near-infrared with the CFHT/WIRCam camera
(Ks band) over an area of 22 and 27 deg2,
respectively. The depth of the photometry was optimised to measure the
physical properties (e.g., star formation rate, stellar masses) of all
the galaxies in the VIPERS spectroscopic survey. The large volume
explored by VIPERS will enable a unique investigation of the
relationship between the galaxy properties and their environment
(density field and cosmic web) at high redshift (0.5 ≤ z ≤ 1.2).
In this paper, we present the observations, the data reductions, and the
build-up of the multi-colour catalogues. The CFHTLS-T0007
(gri-χ2) images are used as reference to detect and
measure the Ks-band photometry, while the T0007
u∗-selected sources are used as priors to perform the
GALEX photometry based on a dedicated software (EMphot). Our final
sample reaches NUVAB {\textasciitilde} 25 (at 5σ) and KAB {\textasciitilde}
22 (at 3σ). The large spectroscopic sample ({\textasciitilde}51 000 spectroscopic
redshifts) allows us to highlight the robustness of our star/galaxy
separation and the reliability of our photometric redshifts with a
typical accuracy of σz ≤ 0.04 and a fraction of
catastrophic failures η ≤ 2\% down to I {\textasciitilde} 23. We present various
tests on the Ks-band completeness and photometric redshift
accuracy by comparing our results with existing overlapping deep
photometric catalogues. Finally, we discuss the BzK sample of passive
and active galaxies at high redshift and the evolution of galaxy
morphology in the (NUV-r) vs. (r-Ks) diagram at low redshift
(z ≤ 0.25) based on the high image quality of the CFHTLS.
The catalogue is available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/590/A102The
images, catalogues, and photometric redshifts for 1.5 million sources
(down to NUV ≤ 25∪Ks ≤ 22) are released and
available at: http://cesam.lam.fr/vipers-mls/},
	urldate = {2018-10-23},
	journal = {A\&A},
	author = {Moutard, T. and Arnouts, S. and Ilbert, O. and Coupon, J. and Hudelot, P. and Vibert, D. and Comte, V. and Conseil, S. and Davidzon, I. and Guzzo, L. and Llebaria, A. and Martin, C. and McCracken, H. J. and Milliard, B. and Morrison, G. and Schiminovich, D. and Treyer, M. and Van Werbaeke, L.},
	month = may,
	year = {2016},
	keywords = {galaxies: photometry, galaxies: distances and redshifts, galaxies: evolution},
	pages = {A102}
}

@article{bielby_wircam_2012,
	title = {The {WIRCam} {Deep} {Survey}. {I}. {Counts}, colours, and mass-functions derived from near-infrared imaging in the {CFHTLS} deep fields},
	volume = {545},
	issn = {0004-6361},
	url = {http://adsabs.harvard.edu/abs/2012A%26A...545A..23B},
	doi = {10.1051/0004-6361/201118547},
	abstract = {We present a new near-infrared imaging survey in the four CFHTLS deep 
fields: the WIRCam Deep Survey or "WIRDS". WIRDS comprises extremely
deep, high quality (FWHM {\textasciitilde} 0.6″) J, H, and Ks imaging
covering a total effective area of 2.1 deg2 and reaching AB
50\% completeness limits of ≈ 24.5. We combine our images with the
CFHTLS to create a unique eight-band ugrizJHKS photometric
catalogues in the four CFHTLS deep fields; these four separate fields
allow us to make a robust estimate of the effect of cosmic variance for
all our measurements. We use these catalogues in combination with ≈
9800 spectroscopic redshifts to estimate precise photometric redshifts
(σΔz/(1 + z) ≲ 0.03 at i {\textless} 25), galaxy
types, star-formation rates and stellar masses for a unique sample of
≈ 1.8 million galaxies. Our JHKs number counts are
consistent with previous studies. We apply the "BzK" selection to our
gzK filter set and find that the star forming BzK selection successfully
selects 76\% of star-forming galaxies in the redshift range 1.4 {\textless} z
{\textless} 2.5 in our photometric catalogue, based on our photometric redshift
measurement. Similarly the passive BzK selection returns 52\% of the
passive 1.4 {\textless} z {\textless} 2.5 population identified in the photometric
catalogue. We present the mass functions of the total galaxy population
as a function of redshift up to z = 2 and present fits using double
Schechter functions. A mass-dependent evolution of the mass function is
seen with the numbers of galaxies with masses of M ≲
1010.75 still evolving at z ≲ 1, but galaxies of higher
mass reaching their present day numbers by z {\textasciitilde} 0.8-1. This is consistent
with the present picture of downsizing in galaxy evolution. We compare
our results with the predictions of the GALFORM semi-analytical galaxy
formation model and find that the simulations provide a relatively
successful fit to the observed mass functions at intermediate masses
(i.e. 10 ≲ log (M/M⊙) ≲ 11). However, as is
common with semi-analytical predictions of the mass function, the
GALFORM results under-predict the mass function at low masses (i.e. log
(M/M⊙) ≲ 10), whilst the fit as a whole degrades
beyondredshifts of z {\textasciitilde} 1.2. All photometric catalogues and images are
made publicly available from TERAPIX and CADC.
Based on observations obtained with MegaPrime/MegaCam, a joint project
of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT)
which is operated by the National Research Council (NRC) of Canada, the
Institut National des Sciences de l'Univers of the Centre National de la
Recherche Scientifique (CNRS) of France, and the University of Hawaii.
This work is based in part on data products produced at TERAPIX and the
Canadian Astronomy Data Centre as part of the Canada-France-Hawaii
Telescope Legacy Survey, a collaborative project of NRC and CNRS.},
	urldate = {2018-10-23},
	journal = {A\&A},
	author = {Bielby, R. and Hudelot, P. and McCracken, H. J. and Ilbert, O. and Daddi, E. and Le Fèvre, O. and Gonzalez-Perez, V. and Kneib, J.-P. and Marmo, C. and Mellier, Y. and Salvato, M. and Sanders, D. B. and Willott, C. J.},
	month = sep,
	year = {2012},
	keywords = {cosmology: observations, mass function, catalogs, galaxies: evolution, galaxies: luminosity function, surveys},
	pages = {A23}
}

@article{leauthaud_weak_2007,
	title = {Weak {Gravitational} {Lensing} with {COSMOS}: {Galaxy} {Selection} and {Shape} {Measurements}},
	volume = {172},
	issn = {0067-0049},
	shorttitle = {Weak {Gravitational} {Lensing} with {COSMOS}},
	url = {https://iopscience.iop.org/article/10.1086/516598/meta},
	doi = {10.1086/516598},
	language = {en},
	number = {1},
	urldate = {2019-07-17},
	journal = {ApJS},
	author = {Leauthaud, Alexie and Massey, Richard and Kneib, Jean-Paul and Rhodes, Jason and Johnston, David E. and Capak, Peter and Heymans, Catherine and Ellis, Richard S. and Koekemoer, Anton M. and Fèvre, Oliver Le and Mellier, Yannick and Réfrégier, Alexandre and Robin, Annie C. and Scoville, Nick and Tasca, Lidia and Taylor, James E. and Waerbeke, Ludovic Van},
	month = sep,
	year = {2007},
	pages = {219}
}

@article{koekemoer_cosmos_2007,
	title = {The {COSMOS} {Survey}: {Hubble} {Space} {Telescope} {Advanced} {Camera} for {Surveys} {Observations} and {Data} {Processing}},
	volume = {172},
	issn = {['0067-0049']},
	shorttitle = {The {COSMOS} {Survey}},
	url = {https://ui.adsabs.harvard.edu/abs/2007ApJS..172..196K/abstract},
	doi = {10.1086/520086},
	abstract = {We describe the details of the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) Wide Field Channel (WFC) observations of the COSMOS field, including the data calibration and processing procedures. We obtained a total of 583 orbits of HST ACS/WFC imaging in the F814W filter, covering a field that is 1.64 deg{\textless}SUP{\textgreater}2{\textless}/SUP{\textgreater} in area, the largest contiguous field ever imaged with HST. The median exposure depth across the field is 2028 s (one HST orbit), achieving a limiting point-source depth AB(F814W)=27.2 (5 σ). We also present details of the astrometric image registration and distortion removal and image combination using MultiDrizzle, motivating the choice of our final pixel scale (30 mas pixel{\textless}SUP{\textgreater}-1{\textless}/SUP{\textgreater}), based on the requirements for weak-lensing science. The final set of images are publicly available through the archive sites at IPAC and STScI, along with further documentation on how they were produced. {\textless}P /{\textgreater}Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy (AURA), Inc., under NASA contract NAS 5-26555 also based on data collected at: the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan; the XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA; the European Southern Observatory under Large Program 175.A-0839, Chile; Kitt Peak National Observatory, Cerro Tololo Inter-American Observatory, and the National Optical Astronomy Observatory, which are operated by AURA under cooperative agreement with the National Science Foundation; the National Radio Astronomy Observatory which is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc; and the Canada-France-Hawaii Telescope (CFHT) with MegaPrime/MegaCam operated as a joint project by the CFHT Corporation, CEA/DAPNIA, the National Research Council of Canada, the Canadian Astronomy Data Centre, the Centre National de la Recherche Scientifique de France, TERAPIX, and the University of Hawaii.},
	language = {en},
	urldate = {2019-11-17},
	journal = {ApJS},
	author = {Koekemoer, A. M. and Aussel, H. and Calzetti, D. and Capak, P. and Giavalisco, M. and Kneib, J.-P. and Leauthaud, A. and Le Fèvre, O. and McCracken, H. J. and Massey, R. and Mobasher, B. and Rhodes, J. and Scoville, N. and Shopbell, P. L.},
	month = sep,
	year = {2007},
	pages = {196}
}

@article{bertin_sextractor:_1996,
	title = {{SExtractor}: {Software} for source extraction.},
	volume = {117},
	issn = {0365-0138},
	shorttitle = {{SExtractor}},
	url = {http://adsabs.harvard.edu/abs/1996A%26AS..117..393B},
	doi = {10.1051/aas:1996164},
	abstract = {We present the automated techniques we have developed for new software that optimally detects, de-blends, measures and classifies sources from astronomical images: SExtractor (Source Extractor). We show that a very reliable star/galaxy separation can be achieved on most images using a neural network trained with simulated images. Salient features of SExtractor include its ability to work on very large images, with minimal human intervention, and to deal with a wide variety of object shapes and magnitudes. It is therefore particularly suited to the analysis of large extragalactic surveys.},
	urldate = {2018-09-29},
	journal = {A\&AS},
	author = {Bertin, E. and Arnouts, S.},
	month = jun,
	year = {1996},
	keywords = {GALAXIES: PHOTOMETRY, METHODS: DATA ANALYSIS, TECHNIQUES: IMAGE PROCESSING},
	pages = {393--404}
}

@INPROCEEDINGS{bertin_terapix_2002,
    author = {{Bertin}, Emmanuel and {Mellier}, Yannick and {Radovich}, Mario and {Missonnier}, Gilles and {Didelon}, Pierre and {Morin}, Bertrand},
    title = "{The TERAPIX Pipeline}",
     keywords = {astronomy: optical, astronomy: software, pipelines: data reduction, software: package, software: development, software: data analysis, data analysis, databases, distributed processing},
    booktitle = {Astronomical Data Analysis Software and Systems XI},
         year = 2002,
       editor = {{Bohlender}, David A. and {Durand}, Daniel and {Handley}, Thomas H.},
       series = {Astronomical Society of the Pacific Conference Series},
       volume = {281},
        month = jan,
        pages = {228},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2002ASPC..281..228B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{kron_photometry_1980,
	title = {Photometry of a complete sample of faint galaxies},
	volume = {43},
	issn = {0067-0049},
	url = {http://adsabs.harvard.edu/abs/1980ApJS...43..305K},
	doi = {10.1086/190669},
	abstract = {Techniques are developed for the automatic measurement of the colors and magnitudes of a complete sample of very faint galaxies. The observations consist of photographic surface photometry in two wavebands for
approximately 20,000 galaxies in two widely separated, high-latitude fields, each having an area of approximately 1080 sq arcmin. The photometric zero points are derived directly from faint stars in the same fields measured photoelectrically by other observers. The
photometry of the galaxy sample is complete to a limit about 10 times fainter than has been systematically investigated before. The sample is characterized by a population of galaxies which becomes bluer with increasing faintness and which increases steeply in number with
increasing faintness in the blue waveband.},
	urldate = {2018-10-23},
	journal = {ApJS},
	author = {Kron, R. G.},
	month = jun,
	year = {1980},
	keywords = {Astronomical Photometry, Calibrating, Colorimetry, Distribution Functions, Galactic Evolution, Galactic Radiation, Galaxies, Luminous Intensity, Star Distribution, Tables (Data)},
	pages = {305--325}
}

@article{arnouts_measuring_2002,
	title = {Measuring the redshift evolution of clustering: the {Hubble} {Deep} {Field} {South}},
	volume = {329},
	issn = {0035-8711},
	shorttitle = {Measuring the redshift evolution of clustering},
	url = {http://adsabs.harvard.edu/abs/2002MNRAS.329..355A},
	doi = {10.1046/j.1365-8711.2002.04988.x},
	abstract = {We present an analysis of the evolution of galaxy clustering in the redshift interval 0{\textless}=z{\textless}=4.5 in the Hubble Deep Field South
(HDF-South). The HST optical data are combined with infrared ISAAC/VLT observations, and photometric redshifts are used for all the galaxies brighter than IAB{\textless}=27.5. The clustering signal is obtained in different redshift bins using two different approaches: a standard one, which uses the best redshift estimate of each object, and a second one, which takes into account the redshift probability function of each object. This second method makes it possible to improve the information in the redshift intervals where contamination from objects with insecure redshifts is important. With both methods, we find that the clustering strength up to z{\textasciitilde}=3.5 in the HDF-South is consistent with the previous results in the HDF-North. Whereas at redshift lower than z{\textasciitilde}1 the HDF galaxy population is un/anti-biased (b{\textless}=1) with respect to the
underlying dark matter, at high redshift the bias increases up to b(z{\textasciitilde}3){\textasciitilde}=2-3, depending on the cosmological model. These results support previous claims that, at high redshift, galaxies are preferentially located in massive haloes, as predicted by the biased galaxy formation scenario. In order to quantify the impact of cosmic errors on our analyses, we have used analytical expressions from Bernstein. Once the behaviour of higher-order moments is assumed, our results show that errors in the clustering measurements in the HDF surveys are indeed dominated by pure shot-noise in most regimes, as assumed in our
analysis. We also show that future observations with instruments like the Advanced Camera on HST will improve the signal-to-noise ratio by at least a factor of 2, as a consequence, more detailed analyses of the errors will be required. In fact, pure shot-noise will give a smaller contribution with respect to other sources of errors, such as finite volume effects or non-Poissonian discreteness effects.},
	urldate = {2018-09-29},
	journal = {MNRAS},
	author = {Arnouts, S. and Moscardini, L. and Vanzella, E. and Colombi, S. and Cristiani, S. and Fontana, A. and Giallongo, E. and Matarrese, S. and Saracco, P.},
	month = jan,
	year = {2002},
	keywords = {COSMOLOGY: OBSERVATIONS, GALAXIES: EVOLUTION, GALAXIES: FORMATION, GALAXIES: HALOES, LARGE-SCALE STRUCTURE OF UNIVERSE},
	pages = {355--366}
}

@article{ilbert_accurate_2006,
	title = {Accurate photometric redshifts for the {CFHT} legacy survey calibrated using the {VIMOS} {VLT} deep survey},
	volume = {457},
	issn = {0004-6361},
	url = {http://adsabs.harvard.edu/abs/2006A%26A...457..841I},
	doi = {10.1051/0004-6361:20065138},
	abstract = {Aims. We present and release photometric redshifts for a uniquely large 
and deep sample of 522286 objects with i'\_AB≤ 25 in the Canada-France
Hawaii Telescope Legacy Survey (CFHTLS) "Deep Survey" fields D1, D2, D3,
and D4, which cover a total effective area of 3.2 °{\textasciicircum}2. 
Methods: . We use 3241 spectroscopic redshifts with 0 ≤ z ≤ 5 from
the VIMOS VLT Deep Survey (VVDS) as a calibration and training set to
derive these photometric redshifts. Using the "Le Phare" photometric
redshift code, we developed a robust calibration method based on an
iterative zero-point refinement combined with a template optimisation
procedure and the application of a Bayesian approach. This method
removes systematic trends in the photometric redshifts and significantly
reduces the fraction of catastrophic errors (by a factor of 2), a
significant improvement over traditional methods. We use our unique
spectroscopic sample to present a detailed assessment of the robustness
of the photometric redshift sample. Results: . For a sample
selected at i'\_AB≤ 24, we reach a redshift accuracy of
σΔ z/(1+z)=0.029 with η=3.8\% of catastrophic
errors (η is defined strictly as those objects with {\textbar}Δ
z{\textbar}/(1+z) {\textgreater} 0.15). The reliability of our photometric redshifts
decreases for faint objects: we find σΔ
z/(1+z)=0.025, 0.034 and η=1.9\%, 5.5\% for samples selected at
i'\_AB=17.5-22.5 and 22.5-24 respectively. We find that the photometric
redshifts of starburst galaxies are less reliable: although these
galaxies represent only 22\% of the spectroscopic sample, they are
responsible for 50\% of the catastrophic errors. An analysis as a
function of redshift demonstrates that our photometric redshifts work
best in the redshift range 0.2≤ z ≤ 1.5. We find an excellent
agreement between the photometric and the VVDS spectroscopic redshift
distributions at i'\_AB≤ 24. Finally, we compare the redshift
distributions of i' selected galaxies on the four CFHTLS deep fields,
showing that cosmic variance is still present on fields of 0.7-0.9
deg{\textasciicircum}2. These photometric redshifts are made publicly available at
http://terapix.iap.fr (complete ascii catalogues) and
http://cencos.oamp.fr/cencos/CFHTLS/ (searchable database interface).},
	urldate = {2018-09-29},
	journal = {A\&A},
	author = {Ilbert, O. and Arnouts, S. and McCracken, H. J. and Bolzonella, M. and Bertin, E. and Le Fèvre, O. and Mellier, Y. and Zamorani, G. and Pellò, R. and Iovino, A. and Tresse, L. and Le Brun, V. and Bottini, D. and Garilli, B. and Maccagni, D. and Picat, J. P. and Scaramella, R. and Scodeggio, M. and Vettolani, G. and Zanichelli, A. and Adami, C. and Bardelli, S. and Cappi, A. and Charlot, S. and Ciliegi, P. and Contini, T. and Cucciati, O. and Foucaud, S. and Franzetti, P. and Gavignaud, I. and Guzzo, L. and Marano, B. and Marinoni, C. and Mazure, A. and Meneux, B. and Merighi, R. and Paltani, S. and Pollo, A. and Pozzetti, L. and Radovich, M. and Zucca, E. and Bondi, M. and Bongiorno, A. and Busarello, G. and de La Torre, S. and Gregorini, L. and Lamareille, F. and Mathez, G. and Merluzzi, P. and Ripepi, V. and Rizzo, D. and Vergani, D.},
	month = oct,
	year = {2006},
	keywords = {galaxies: photometry, galaxies: distances and redshifts, methods: data analysis},
	pages = {841--856}
}

@ARTICLE{ilbert_photoz_2009,
       author = {{Ilbert}, O. and {Capak}, P. and {Salvato}, M. and {Aussel}, H. and
         {McCracken}, H.~J. and {Sanders}, D.~B. and {Scoville}, N. and
         {Kartaltepe}, J. and {Arnouts}, S. and {Le Floc'h}, E. and
         {Mobasher}, B. and {Taniguchi}, Y. and {Lamareille}, F. and
         {Leauthaud}, A. and {Sasaki}, S. and {Thompson}, D. and {Zamojski}, M. and
         {Zamorani}, G. and {Bardelli}, S. and {Bolzonella}, M. and
         {Bongiorno}, A. and {Brusa}, M. and {Caputi}, K.~I. and
         {Carollo}, C.~M. and {Contini}, T. and {Cook}, R. and {Coppa}, G. and
         {Cucciati}, O. and {de la Torre}, S. and {de Ravel}, L. and
         {Franzetti}, P. and {Garilli}, B. and {Hasinger}, G. and {Iovino}, A. and
         {Kampczyk}, P. and {Kneib}, J. -P. and {Knobel}, C. and {Kovac}, K. and
         {Le Borgne}, J.~F. and {Le Brun}, V. and {Le F{\`e}vre}, O. and
         {Lilly}, S. and {Looper}, D. and {Maier}, C. and {Mainieri}, V. and
         {Mellier}, Y. and {Mignoli}, M. and {Murayama}, T. and {Pell{\`o}}, R. and
         {Peng}, Y. and {P{\'e}rez-Montero}, E. and {Renzini}, A. and
         {Ricciardelli}, E. and {Schiminovich}, D. and {Scodeggio}, M. and
         {Shioya}, Y. and {Silverman}, J. and {Surace}, J. and {Tanaka}, M. and
         {Tasca}, L. and {Tresse}, L. and {Vergani}, D. and {Zucca}, E.},
        title = "{Cosmos Photometric Redshifts with 30-Bands for 2-deg$^{2}$}",
      journal = {\apj},
     keywords = {galaxies: distances and redshifts, galaxies: evolution, galaxies: formation, Astrophysics},
         year = 2009,
        month = jan,
       volume = {690},
       number = {2},
        pages = {1236-1249},
          doi = {10.1088/0004-637X/690/2/1236},
archivePrefix = {arXiv},
       eprint = {0809.2101},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009ApJ...690.1236I},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@article{gaia_collaboration_gaia_2016,
	title = {\textit{{Gaia}} {Data} {Release} 1: {Summary} of the astrometric, photometric, and survey properties},
	volume = {595},
	issn = {0004-6361, 1432-0746},
	shorttitle = {\textit{{Gaia}} {Data} {Release} 1},
	url = {http://www.aanda.org/10.1051/0004-6361/201629512},
	doi = {10.1051/0004-6361/201629512},
	abstract = {Methods. The raw data collected by Gaia during the ﬁrst 14 months of the mission have been processed by the Gaia Data Processing and Analysis Consortium (DPAC) and turned into an astrometric and photometric catalogue.
Results. Gaia DR1 consists of three components: a primary astrometric data set which contains the positions, parallaxes, and mean proper motions for about 2 million of the brightest stars in common with the Hipparcos and Tycho-2 catalogues – a realisation of the Tycho-Gaia Astrometric Solution (TGAS) – and a secondary astrometric data set containing the positions for an additional 1.1 billion sources. The second component is the photometric data set, consisting of mean G-band magnitudes for all sources. The G-band light curves and the characteristics of ∼3000 Cepheid and RR Lyrae stars, observed at high cadence around the south ecliptic pole, form the third component. For the primary astrometric data set the typical uncertainty is about 0.3 mas for the positions and parallaxes, and about 1 mas yr−1 for the proper motions. A systematic component of ∼0.3 mas should be added to the parallax uncertainties. For the subset of ∼94 000 Hipparcos stars in the primary data set, the proper motions are much more precise at about 0.06 mas yr−1. For the secondary astrometric data set, the typical uncertainty of the positions is ∼10 mas. The median uncertainties on the mean G-band magnitudes range from the mmag level to ∼0.03 mag over the magnitude range 5 to 20.7.
Conclusions. Gaia DR1 is an important milestone ahead of the next Gaia data release, which will feature ﬁve-parameter astrometry for all sources. Extensive validation shows that Gaia DR1 represents a major advance in the mapping of the heavens and the availability of basic stellar data that underpin observational astrophysics. Nevertheless, the very preliminary nature of this ﬁrst Gaia data release does lead to a number of important limitations to the data quality which should be carefully considered before drawing conclusions from the data.},
	language = {en},
	urldate = {2019-02-12},
	journal = {Astronomy \& Astrophysics},
	author = {{Gaia Collaboration} and Brown, A. G. A. and Vallenari, A. and Prusti, T. and de Bruijne, J. H.J. and Mignard, F. and Drimmel, R. and Babusiaux, C. and Bailer-Jones, C. A.L. and Bastian, U. and Biermann, M. and Evans, D. W. and Eyer, L. and Jansen, F. and Jordi, C. and Katz, D. and Klioner, S. A. and Lammers, U. and Lindegren, L. and Luri, X. and O’Mullane, W. and Panem, C. and Pourbaix, D. and Randich, S. and Sartoretti, P. and Siddiqui, H. I. and Soubiran, C. and Valette, V. and van Leeuwen, F. and Walton, N. A. and Aerts, C. and Arenou, F. and Cropper, M. and Høg, E. and Lattanzi, M. G. and Grebel, E. K. and Holland, A. D. and Huc, C. and Passot, X. and Perryman, M. and Bramante, L. and Cacciari, C. and Castañeda, J. and Chaoul, L. and Cheek, N. and De Angeli, F. and Fabricius, C. and Guerra, R. and Hernández, J. and Jean-Antoine-Piccolo, A. and Masana, E. and Messineo, R. and Mowlavi, N. and Nienartowicz, K. and Ordóñez-Blanco, D. and Panuzzo, P. and Portell, J. and Richards, P. J. and Riello, M. and Seabroke, G. M. and Tanga, P. and Thévenin, F. and Torra, J. and Els, S. G. and Gracia-Abril, G. and Comoretto, G. and Garcia-Reinaldos, M. and Lock, T. and Mercier, E. and Altmann, M. and Andrae, R. and Astraatmadja, T. L. and Bellas-Velidis, I. and Benson, K. and Berthier, J. and Blomme, R. and Busso, G. and Carry, B. and Cellino, A. and Clementini, G. and Cowell, S. and Creevey, O. and Cuypers, J. and Davidson, M. and De Ridder, J. and de Torres, A. and Delchambre, L. and Dell’Oro, A. and Ducourant, C. and Frémat, Y. and García-Torres, M. and Gosset, E. and Halbwachs, J.-L. and Hambly, N. C. and Harrison, D. L. and Hauser, M. and Hestroffer, D. and Hodgkin, S. T. and Huckle, H. E. and Hutton, A. and Jasniewicz, G. and Jordan, S. and Kontizas, M. and Korn, A. J. and Lanzafame, A. C. and Manteiga, M. and Moitinho, A. and Muinonen, K. and Osinde, J. and Pancino, E. and Pauwels, T. and Petit, J.-M. and Recio-Blanco, A. and Robin, A. C. and Sarro, L. M. and Siopis, C. and Smith, M. and Smith, K. W. and Sozzetti, A. and Thuillot, W. and van Reeven, W. and Viala, Y. and Abbas, U. and Abreu Aramburu, A. and Accart, S. and Aguado, J. J. and Allan, P. M. and Allasia, W. and Altavilla, G. and Álvarez, M. A. and Alves, J. and Anderson, R. I. and Andrei, A. H. and Anglada Varela, E. and Antiche, E. and Antoja, T. and Antón, S. and Arcay, B. and Bach, N. and Baker, S. G. and Balaguer-Núñez, L. and Barache, C. and Barata, C. and Barbier, A. and Barblan, F. and Barrado y Navascués, D. and Barros, M. and Barstow, M. A. and Becciani, U. and Bellazzini, M. and Bello García, A. and Belokurov, V. and Bendjoya, P. and Berihuete, A. and Bianchi, L. and Bienaymé, O. and Billebaud, F. and Blagorodnova, N. and Blanco-Cuaresma, S. and Boch, T. and Bombrun, A. and Borrachero, R. and Bouquillon, S. and Bourda, G. and Bouy, H. and Bragaglia, A. and Breddels, M. A. and Brouillet, N. and Brüsemeister, T. and Bucciarelli, B. and Burgess, P. and Burgon, R. and Burlacu, A. and Busonero, D. and Buzzi, R. and Caffau, E. and Cambras, J. and Campbell, H. and Cancelliere, R. and Cantat-Gaudin, T. and Carlucci, T. and Carrasco, J. M. and Castellani, M. and Charlot, P. and Charnas, J. and Chiavassa, A. and Clotet, M. and Cocozza, G. and Collins, R. S. and Costigan, G. and Crifo, F. and Cross, N. J.G. and Crosta, M. and Crowley, C. and Dafonte, C. and Damerdji, Y. and Dapergolas, A. and David, P. and David, M. and De Cat, P. and de Felice, F. and de Laverny, P. and De Luise, F. and De March, R. and de Martino, D. and de Souza, R. and Debosscher, J. and del Pozo, E. and Delbo, M. and Delgado, A. and Delgado, H. E. and Di Matteo, P. and Diakite, S. and Distefano, E. and Dolding, C. and Dos Anjos, S. and Drazinos, P. and Duran, J. and Dzigan, Y. and Edvardsson, B. and Enke, H. and Evans, N. W. and Eynard Bontemps, G. and Fabre, C. and Fabrizio, M. and Faigler, S. and Falcão, A. J. and Farràs Casas, M. and Federici, L. and Fedorets, G. and Fernández-Hernández, J. and Fernique, P. and Fienga, A. and Figueras, F. and Filippi, F. and Findeisen, K. and Fonti, A. and Fouesneau, M. and Fraile, E. and Fraser, M. and Fuchs, J. and Gai, M. and Galleti, S. and Galluccio, L. and Garabato, D. and García-Sedano, F. and Garofalo, A. and Garralda, N. and Gavras, P. and Gerssen, J. and Geyer, R. and Gilmore, G. and Girona, S. and Giuffrida, G. and Gomes, M. and González-Marcos, A. and González-Núñez, J. and González-Vidal, J. J. and Granvik, M. and Guerrier, A. and Guillout, P. and Guiraud, J. and Gúrpide, A. and Gutiérrez-Sánchez, R. and Guy, L. P. and Haigron, R. and Hatzidimitriou, D. and Haywood, M. and Heiter, U. and Helmi, A. and Hobbs, D. and Hofmann, W. and Holl, B. and Holland, G. and Hunt, J. A.S. and Hypki, A. and Icardi, V. and Irwin, M. and Jevardat de Fombelle, G. and Jofré, P. and Jonker, P. G. and Jorissen, A. and Julbe, F. and Karampelas, A. and Kochoska, A. and Kohley, R. and Kolenberg, K. and Kontizas, E. and Koposov, S. E. and Kordopatis, G. and Koubsky, P. and Krone-Martins, A. and Kudryashova, M. and Kull, I. and Bachchan, R. K. and Lacoste-Seris, F. and Lanza, A. F. and Lavigne, J.-B. and Le Poncin-Lafitte, C. and Lebreton, Y. and Lebzelter, T. and Leccia, S. and Leclerc, N. and Lecoeur-Taibi, I. and Lemaitre, V. and Lenhardt, H. and Leroux, F. and Liao, S. and Licata, E. and Lindstrøm, H. E.P. and Lister, T. A. and Livanou, E. and Lobel, A. and Löffler, W. and López, M. and Lorenz, D. and MacDonald, I. and Magalhães Fernandes, T. and Managau, S. and Mann, R. G. and Mantelet, G. and Marchal, O. and Marchant, J. M. and Marconi, M. and Marinoni, S. and Marrese, P. M. and Marschalkó, G. and Marshall, D. J. and Martín-Fleitas, J. M. and Martino, M. and Mary, N. and Matijevič, G. and Mazeh, T. and McMillan, P. J. and Messina, S. and Michalik, D. and Millar, N. R. and Miranda, B. M. H. and Molina, D. and Molinaro, R. and Molinaro, M. and Molnár, L. and Moniez, M. and Montegriffo, P. and Mor, R. and Mora, A. and Morbidelli, R. and Morel, T. and Morgenthaler, S. and Morris, D. and Mulone, A. F. and Muraveva, T. and Musella, I. and Narbonne, J. and Nelemans, G. and Nicastro, L. and Noval, L. and Ordénovic, C. and Ordieres-Meré, J. and Osborne, P. and Pagani, C. and Pagano, I. and Pailler, F. and Palacin, H. and Palaversa, L. and Parsons, P. and Pecoraro, M. and Pedrosa, R. and Pentikäinen, H. and Pichon, B. and Piersimoni, A. M. and Pineau, F.-X. and Plachy, E. and Plum, G. and Poujoulet, E. and Prša, A. and Pulone, L. and Ragaini, S. and Rago, S. and Rambaux, N. and Ramos-Lerate, M. and Ranalli, P. and Rauw, G. and Read, A. and Regibo, S. and Reylé, C. and Ribeiro, R. A. and Rimoldini, L. and Ripepi, V. and Riva, A. and Rixon, G. and Roelens, M. and Romero-Gómez, M. and Rowell, N. and Royer, F. and Ruiz-Dern, L. and Sadowski, G. and Sagristà Sellés, T. and Sahlmann, J. and Salgado, J. and Salguero, E. and Sarasso, M. and Savietto, H. and Schultheis, M. and Sciacca, E. and Segol, M. and Segovia, J. C. and Segransan, D. and Shih, I.-C. and Smareglia, R. and Smart, R. L. and Solano, E. and Solitro, F. and Sordo, R. and Soria Nieto, S. and Souchay, J. and Spagna, A. and Spoto, F. and Stampa, U. and Steele, I. A. and Steidelmüller, H. and Stephenson, C. A. and Stoev, H. and Suess, F. F. and Süveges, M. and Surdej, J. and Szabados, L. and Szegedi-Elek, E. and Tapiador, D. and Taris, F. and Tauran, G. and Taylor, M. B. and Teixeira, R. and Terrett, D. and Tingley, B. and Trager, S. C. and Turon, C. and Ulla, A. and Utrilla, E. and Valentini, G. and van Elteren, A. and Van Hemelryck, E. and van Leeuwen, M. and Varadi, M. and Vecchiato, A. and Veljanoski, J. and Via, T. and Vicente, D. and Vogt, S. and Voss, H. and Votruba, V. and Voutsinas, S. and Walmsley, G. and Weiler, M. and Weingrill, K. and Wevers, T. and Wyrzykowski, Ł. and Yoldas, A. and Žerjal, M. and Zucker, S. and Zurbach, C. and Zwitter, T. and Alecu, A. and Allen, M. and Allende Prieto, C. and Amorim, A. and Anglada-Escudé, G. and Arsenijevic, V. and Azaz, S. and Balm, P. and Beck, M. and Bernstein, H.-H. and Bigot, L. and Bijaoui, A. and Blasco, C. and Bonfigli, M. and Bono, G. and Boudreault, S. and Bressan, A. and Brown, S. and Brunet, P.-M. and Bunclark, P. and Buonanno, R. and Butkevich, A. G. and Carret, C. and Carrion, C. and Chemin, L. and Chéreau, F. and Corcione, L. and Darmigny, E. and de Boer, K. S. and de Teodoro, P. and de Zeeuw, P. T. and Delle Luche, C. and Domingues, C. D. and Dubath, P. and Fodor, F. and Frézouls, B. and Fries, A. and Fustes, D. and Fyfe, D. and Gallardo, E. and Gallegos, J. and Gardiol, D. and Gebran, M. and Gomboc, A. and Gómez, A. and Grux, E. and Gueguen, A. and Heyrovsky, A. and Hoar, J. and Iannicola, G. and Isasi Parache, Y. and Janotto, A.-M. and Joliet, E. and Jonckheere, A. and Keil, R. and Kim, D.-W. and Klagyivik, P. and Klar, J. and Knude, J. and Kochukhov, O. and Kolka, I. and Kos, J. and Kutka, A. and Lainey, V. and LeBouquin, D. and Liu, C. and Loreggia, D. and Makarov, V. V. and Marseille, M. G. and Martayan, C. and Martinez-Rubi, O. and Massart, B. and Meynadier, F. and Mignot, S. and Munari, U. and Nguyen, A.-T. and Nordlander, T. and Ocvirk, P. and O’Flaherty, K. S. and Olias Sanz, A. and Ortiz, P. and Osorio, J. and Oszkiewicz, D. and Ouzounis, A. and Palmer, M. and Park, P. and Pasquato, E. and Peltzer, C. and Peralta, J. and Péturaud, F. and Pieniluoma, T. and Pigozzi, E. and Poels, J. and Prat, G. and Prod’homme, T. and Raison, F. and Rebordao, J. M. and Risquez, D. and Rocca-Volmerange, B. and Rosen, S. and Ruiz-Fuertes, M. I. and Russo, F. and Sembay, S. and Serraller Vizcaino, I. and Short, A. and Siebert, A. and Silva, H. and Sinachopoulos, D. and Slezak, E. and Soffel, M. and Sosnowska, D. and Straižys, V. and ter Linden, M. and Terrell, D. and Theil, S. and Tiede, C. and Troisi, L. and Tsalmantza, P. and Tur, D. and Vaccari, M. and Vachier, F. and Valles, P. and Van Hamme, W. and Veltz, L. and Virtanen, J. and Wallut, J.-M. and Wichmann, R. and Wilkinson, M. I. and Ziaeepour, H. and Zschocke, S.},
	month = nov,
	year = {2016},
	pages = {A2}
}

@article{gaia_collaboration_gaia_2018,
	title = {\textit{{Gaia}} {Data} {Release} 2: {Summary} of the contents and survey properties},
	volume = {616},
	issn = {0004-6361, 1432-0746},
	shorttitle = {\textit{{Gaia}} {Data} {Release} 2},
	url = {https://www.aanda.org/10.1051/0004-6361/201833051},
	doi = {10.1051/0004-6361/201833051},
	abstract = {Methods. The raw data collected with the Gaia instruments during the ﬁrst 22 months of the mission have been processed by the Gaia Data Processing and Analysis Consortium (DPAC) and turned into this second data release, which represents a major advance with respect to Gaia DR1 in terms of completeness, performance, and richness of the data products.
Results. Gaia DR2 contains celestial positions and the apparent brightness in G for approximately 1.7 billion sources. For 1.3 billion of those sources, parallaxes and proper motions are in addition available. The sample of sources for which variability information is provided is expanded to 0.5 million stars. This data release contains four new elements: broad-band colour information in the form of the apparent brightness in the GBP (330–680 nm) and GRP (630–1050 nm) bands is available for 1.4 billion sources; median radial velocities for some 7 million sources are presented; for between 77 and 161 million sources estimates are provided of the stellar effective temperature, extinction, reddening, and radius and luminosity; and for a pre-selected list of 14 000 minor planets in the solar system epoch astrometry and photometry are presented. Finally, Gaia DR2 also represents a new materialisation of the celestial reference frame in the optical, the Gaia-CRF2, which is the ﬁrst optical reference frame based solely on extragalactic sources. There are notable changes in the photometric system and the catalogue source list with respect to Gaia DR1, and we stress the need to consider the two data releases as independent.
Conclusions. Gaia DR2 represents a major achievement for the Gaia mission, delivering on the long standing promise to provide parallaxes and proper motions for over 1 billion stars, and representing a ﬁrst step in the availability of complementary radial velocity and source astrophysical information for a sample of stars in the Gaia survey which covers a very substantial fraction of the volume of our galaxy.},
	language = {en},
	urldate = {2020-03-11},
	journal = {Astronomy \& Astrophysics},
	author = {{Gaia Collaboration} and Brown, A. G. A. and Vallenari, A. and Prusti, T. and de Bruijne, J. H. J. and Babusiaux, C. and Bailer-Jones, C. A. L. and Biermann, M. and Evans, D. W. and Eyer, L. and Jansen, F. and Jordi, C. and Klioner, S. A. and Lammers, U. and Lindegren, L. and Luri, X. and Mignard, F. and Panem, C. and Pourbaix, D. and Randich, S. and Sartoretti, P. and Siddiqui, H. I. and Soubiran, C. and van Leeuwen, F. and Walton, N. A. and Arenou, F. and Bastian, U. and Cropper, M. and Drimmel, R. and Katz, D. and Lattanzi, M. G. and Bakker, J. and Cacciari, C. and Castañeda, J. and Chaoul, L. and Cheek, N. and De Angeli, F. and Fabricius, C. and Guerra, R. and Holl, B. and Masana, E. and Messineo, R. and Mowlavi, N. and Nienartowicz, K. and Panuzzo, P. and Portell, J. and Riello, M. and Seabroke, G. M. and Tanga, P. and Thévenin, F. and Gracia-Abril, G. and Comoretto, G. and Garcia-Reinaldos, M. and Teyssier, D. and Altmann, M. and Andrae, R. and Audard, M. and Bellas-Velidis, I. and Benson, K. and Berthier, J. and Blomme, R. and Burgess, P. and Busso, G. and Carry, B. and Cellino, A. and Clementini, G. and Clotet, M. and Creevey, O. and Davidson, M. and De Ridder, J. and Delchambre, L. and Dell’Oro, A. and Ducourant, C. and Fernández-Hernández, J. and Fouesneau, M. and Frémat, Y. and Galluccio, L. and García-Torres, M. and González-Núñez, J. and González-Vidal, J. J. and Gosset, E. and Guy, L. P. and Halbwachs, J.-L. and Hambly, N. C. and Harrison, D. L. and Hernández, J. and Hestroffer, D. and Hodgkin, S. T. and Hutton, A. and Jasniewicz, G. and Jean-Antoine-Piccolo, A. and Jordan, S. and Korn, A. J. and Krone-Martins, A. and Lanzafame, A. C. and Lebzelter, T. and Löffler, W. and Manteiga, M. and Marrese, P. M. and Martín-Fleitas, J. M. and Moitinho, A. and Mora, A. and Muinonen, K. and Osinde, J. and Pancino, E. and Pauwels, T. and Petit, J.-M. and Recio-Blanco, A. and Richards, P. J. and Rimoldini, L. and Robin, A. C. and Sarro, L. M. and Siopis, C. and Smith, M. and Sozzetti, A. and Süveges, M. and Torra, J. and van Reeven, W. and Abbas, U. and Abreu Aramburu, A. and Accart, S. and Aerts, C. and Altavilla, G. and Álvarez, M. A. and Alvarez, R. and Alves, J. and Anderson, R. I. and Andrei, A. H. and Anglada Varela, E. and Antiche, E. and Antoja, T. and Arcay, B. and Astraatmadja, T. L. and Bach, N. and Baker, S. G. and Balaguer-Núñez, L. and Balm, P. and Barache, C. and Barata, C. and Barbato, D. and Barblan, F. and Barklem, P. S. and Barrado, D. and Barros, M. and Barstow, M. A. and Bartholomé Muñoz, S. and Bassilana, J.-L. and Becciani, U. and Bellazzini, M. and Berihuete, A. and Bertone, S. and Bianchi, L. and Bienaymé, O. and Blanco-Cuaresma, S. and Boch, T. and Boeche, C. and Bombrun, A. and Borrachero, R. and Bossini, D. and Bouquillon, S. and Bourda, G. and Bragaglia, A. and Bramante, L. and Breddels, M. A. and Bressan, A. and Brouillet, N. and Brüsemeister, T. and Brugaletta, E. and Bucciarelli, B. and Burlacu, A. and Busonero, D. and Butkevich, A. G. and Buzzi, R. and Caffau, E. and Cancelliere, R. and Cannizzaro, G. and Cantat-Gaudin, T. and Carballo, R. and Carlucci, T. and Carrasco, J. M. and Casamiquela, L. and Castellani, M. and Castro-Ginard, A. and Charlot, P. and Chemin, L. and Chiavassa, A. and Cocozza, G. and Costigan, G. and Cowell, S. and Crifo, F. and Crosta, M. and Crowley, C. and Cuypers†, J. and Dafonte, C. and Damerdji, Y. and Dapergolas, A. and David, P. and David, M. and de Laverny, P. and De Luise, F. and De March, R. and de Martino, D. and de Souza, R. and de Torres, A. and Debosscher, J. and del Pozo, E. and Delbo, M. and Delgado, A. and Delgado, H. E. and Di Matteo, P. and Diakite, S. and Diener, C. and Distefano, E. and Dolding, C. and Drazinos, P. and Durán, J. and Edvardsson, B. and Enke, H. and Eriksson, K. and Esquej, P. and Eynard Bontemps, G. and Fabre, C. and Fabrizio, M. and Faigler, S. and Falcão, A. J. and Farràs Casas, M. and Federici, L. and Fedorets, G. and Fernique, P. and Figueras, F. and Filippi, F. and Findeisen, K. and Fonti, A. and Fraile, E. and Fraser, M. and Frézouls, B. and Gai, M. and Galleti, S. and Garabato, D. and García-Sedano, F. and Garofalo, A. and Garralda, N. and Gavel, A. and Gavras, P. and Gerssen, J. and Geyer, R. and Giacobbe, P. and Gilmore, G. and Girona, S. and Giuffrida, G. and Glass, F. and Gomes, M. and Granvik, M. and Gueguen, A. and Guerrier, A. and Guiraud, J. and Gutiérrez-Sánchez, R. and Haigron, R. and Hatzidimitriou, D. and Hauser, M. and Haywood, M. and Heiter, U. and Helmi, A. and Heu, J. and Hilger, T. and Hobbs, D. and Hofmann, W. and Holland, G. and Huckle, H. E. and Hypki, A. and Icardi, V. and Janßen, K. and Jevardat de Fombelle, G. and Jonker, P. G. and Juhász, Á. L. and Julbe, F. and Karampelas, A. and Kewley, A. and Klar, J. and Kochoska, A. and Kohley, R. and Kolenberg, K. and Kontizas, M. and Kontizas, E. and Koposov, S. E. and Kordopatis, G. and Kostrzewa-Rutkowska, Z. and Koubsky, P. and Lambert, S. and Lanza, A. F. and Lasne, Y. and Lavigne, J.-B. and Le Fustec, Y. and Le Poncin-Lafitte, C. and Lebreton, Y. and Leccia, S. and Leclerc, N. and Lecoeur-Taibi, I. and Lenhardt, H. and Leroux, F. and Liao, S. and Licata, E. and Lindstrøm, H. E. P. and Lister, T. A. and Livanou, E. and Lobel, A. and López, M. and Managau, S. and Mann, R. G. and Mantelet, G. and Marchal, O. and Marchant, J. M. and Marconi, M. and Marinoni, S. and Marschalkó, G. and Marshall, D. J. and Martino, M. and Marton, G. and Mary, N. and Massari, D. and Matijevič, G. and Mazeh, T. and McMillan, P. J. and Messina, S. and Michalik, D. and Millar, N. R. and Molina, D. and Molinaro, R. and Molnár, L. and Montegriffo, P. and Mor, R. and Morbidelli, R. and Morel, T. and Morris, D. and Mulone, A. F. and Muraveva, T. and Musella, I. and Nelemans, G. and Nicastro, L. and Noval, L. and O’Mullane, W. and Ordénovic, C. and Ordóñez-Blanco, D. and Osborne, P. and Pagani, C. and Pagano, I. and Pailler, F. and Palacin, H. and Palaversa, L. and Panahi, A. and Pawlak, M. and Piersimoni, A. M. and Pineau, F.-X. and Plachy, E. and Plum, G. and Poggio, E. and Poujoulet, E. and Prša, A. and Pulone, L. and Racero, E. and Ragaini, S. and Rambaux, N. and Ramos-Lerate, M. and Regibo, S. and Reylé, C. and Riclet, F. and Ripepi, V. and Riva, A. and Rivard, A. and Rixon, G. and Roegiers, T. and Roelens, M. and Romero-Gómez, M. and Rowell, N. and Royer, F. and Ruiz-Dern, L. and Sadowski, G. and Sagristà Sellés, T. and Sahlmann, J. and Salgado, J. and Salguero, E. and Sanna, N. and Santana-Ros, T. and Sarasso, M. and Savietto, H. and Schultheis, M. and Sciacca, E. and Segol, M. and Segovia, J. C. and Ségransan, D. and Shih, I-C. and Siltala, L. and Silva, A. F. and Smart, R. L. and Smith, K. W. and Solano, E. and Solitro, F. and Sordo, R. and Soria Nieto, S. and Souchay, J. and Spagna, A. and Spoto, F. and Stampa, U. and Steele, I. A. and Steidelmüller, H. and Stephenson, C. A. and Stoev, H. and Suess, F. F. and Surdej, J. and Szabados, L. and Szegedi-Elek, E. and Tapiador, D. and Taris, F. and Tauran, G. and Taylor, M. B. and Teixeira, R. and Terrett, D. and Teyssandier, P. and Thuillot, W. and Titarenko, A. and Torra Clotet, F. and Turon, C. and Ulla, A. and Utrilla, E. and Uzzi, S. and Vaillant, M. and Valentini, G. and Valette, V. and van Elteren, A. and Van Hemelryck, E. and van Leeuwen, M. and Vaschetto, M. and Vecchiato, A. and Veljanoski, J. and Viala, Y. and Vicente, D. and Vogt, S. and von Essen, C. and Voss, H. and Votruba, V. and Voutsinas, S. and Walmsley, G. and Weiler, M. and Wertz, O. and Wevers, T. and Wyrzykowski, Ł. and Yoldas, A. and Žerjal, M. and Ziaeepour, H. and Zorec, J. and Zschocke, S. and Zucker, S. and Zurbach, C. and Zwitter, T.},
	month = aug,
	year = {2018},
	pages = {A1}
}

@article{zamojski_deep_2007,
	title = {Deep {GALEX} {Imaging} of the {COSMOS} {HST} {Field}: {A} {First} {Look} at the {Morphology} of z {\textasciitilde} 0.7 {Star}-forming {Galaxies}},
	volume = {172},
	issn = {0067-0049},
	shorttitle = {Deep {GALEX} {Imaging} of the {COSMOS} {HST} {Field}},
	url = {http://adsabs.harvard.edu/abs/2007ApJS..172..468Z},
	doi = {10.1086/516593},
	abstract = {We present a study of the morphological nature of redshift z{\textasciitilde}0.7 
star-forming galaxies using a combination of HST ACS, GALEX, and
ground-based images of the COSMOS field. Our sample consists of 8146
galaxies, 5777 of which are detected in the GALEX near-ultraviolet band
(2310 Å or {\textasciitilde}1360 Å rest frame) down to a limiting magnitude
of 25.5 (AB), and all of which have a brightness of F814W(HST){\textless}23 mag
and photometric redshifts in the range 0.5520). We observe a bimodality
in the galaxy population in asymmetry and in clumpiness, although the
separation is most evident when either of those parameters is combined
with a concentration-like parameter (C, G, or M20). We
further show that this morphological bimodality has a strong
correspondence with the FUV-g color bimodality and conclude that
UV-optical color predominantly evolves concurrently with morphology. We
observe many of the most star-forming galaxies to have morphologies
approaching that of early-type galaxies, and we interpret this as
evidence that strong starburst events are linked to bulge growth and
constitute a process through which galaxies can be brought from the blue
to the red sequence while simultaneously modifying their morphology
accordingly. We conclude that the red sequence has continued growing at
z{\textless}{\textasciitilde}0.7. We also observe z{\textasciitilde}0.7 galaxies to have physical properties
similar to that of local galaxies, except for higher star formation
rates. Whence we infer that the dimming of star-forming galaxies is
responsible for most of the evolution in star formation rate density
since that redshift, although our data are also consistent with a mild
number evolution.

Based on observations with the NASA/ESA Hubble Space Telescope, obtained
at the Space Telescope Science Institute, which is operated by
Association of Universities for Research in Astronomy, Inc. (AURA),
under NASA contract NAS 5-26555 and with the NASA Galaxy Evolution
Explorer (GALEX); also based on data collected at the Subaru Telescope,
which is operated by the National Astronomical Observatory of Japan;
Kitt Peak National Observatory, Cerro Tololo Inter-American Observatory,
and the National Optical Astronomy Observatory, which are operated by
the Association of Universities for Research in Astronomy, Inc. (AURA),
under cooperative agreement with the National Science Foundation; the
Canada-France-Hawaii Telescope with MegaPrime/MegaCam operated as a
joint project by the CFHT Corporation, CEA/DAPNIA, the National Research
Council of Canada, the Canadian Astronomy Data Centre, the Centre
National de la Recherche Scientifique de France, TERAPIX, and the
University of Hawaii.},
	urldate = {2020-05-08},
	journal = {The Astrophysical Journal Supplement Series},
	author = {Zamojski, M. A. and Schiminovich, D. and Rich, R. M. and Mobasher, B. and Koekemoer, A. M. and Capak, P. and Taniguchi, Y. and Sasaki, S. S. and McCracken, H. J. and Mellier, Y. and Bertin, E. and Aussel, H. and Sanders, D. B. and Le Fèvre, O. and Ilbert, O. and Salvato, M. and Thompson, D. J. and Kartaltepe, J. S. and Scoville, N. and Barlow, T. A. and Forster, K. and Friedman, P. G. and Martin, D. C. and Morrissey, P. and Neff, S. G. and Seibert, M. and Small, T. and Wyder, T. K. and Bianchi, L. and Donas, J. and Heckman, T. M. and Lee, Y.-W. and Madore, B. F. and Milliard, B. and Szalay, A. S. and Welsh, B. Y. and Yi, S. K.},
	month = sep,
	year = {2007},
	keywords = {Galaxies: Evolution, Galaxies: Fundamental Parameters, Surveys},
	pages = {468--493}
}

@article{aihara_second_2019,
	title = {Second data release of the {Hyper} {Suprime}-{Cam} {Subaru} {Strategic} {Program}},
	volume = {71},
	issn = {0004-6264},
	url = {http://adsabs.harvard.edu/abs/2019PASJ...71..114A},
	doi = {10.1093/pasj/psz103},
	abstract = {This paper presents the second data release of the Hyper Suprime-Cam Subaru Strategic Program, a wide-field optical imaging survey using the 8.2 m Subaru Telescope. The release includes data from 174 nights of observation through 2018 January. The Wide layer data cover about 300 deg{\textasciicircum}2 in all five broad-band filters (grizy) to the nominal survey exposure (10 min in gr and 20 min in izy). Partially observed areas are also included in the release; about 1100 deg{\textasciicircum}2 is observed in at least one filter and one exposure. The median seeing in the i-band is
\{0.{\textasciicircum}' ' \vphantom{\{}\}6\}, demonstrating the superb image quality of the survey. The Deep (26 deg{\textasciicircum}2) and UltraDeep (4 deg{\textasciicircum}2) data are jointly processed and the UltraDeep-COSMOS field reaches an unprecedented depth of i∼ 28 at 5 σ for point sources. In addition to the
broad-band data, narrow-band data are also available in the Deep and UltraDeep fields. This release includes a major update to the processing pipeline, including improved sky subtraction, PSF modeling, object detection, and artifact rejection. The overall data quality has been improved, but this release is not without problems; there is a
persistent deblender problem as well as new issues with masks around bright stars. The user is encouraged to review the issue list before utilizing the data for scientific explorations. All the image products as well as catalog products are available for download. The catalogs are also loaded into a database, which provides an easy interface for users to retrieve data for objects of interest. In addition to these main data products, detailed galaxy shape measurements withheld from Public Data Release 1 (PDR1) are now available to the community. The shape catalog is drawn from the S16A internal release, which has a larger area than PDR1 (160 deg{\textasciicircum}2). All products are available at the data release site, https://hsc-release.mtk.nao.ac.jp/.},
	urldate = {2020-05-08},
	journal = {Publications of the Astronomical Society of Japan},
	author = {Aihara, Hiroaki and AlSayyad, Yusra and Ando, Makoto and Armstrong, Robert and Bosch, James and Egami, Eiichi and Furusawa, Hisanori and Furusawa, Junko and Goulding, Andy and Harikane, Yuichi and Hikage, Chiaki and Ho, Paul T. P. and Hsieh, Bau-Ching and Huang, Song and Ikeda, Hiroyuki and Imanishi, Masatoshi and Ito, Kei and Iwata, Ikuru and Jaelani, Anton T. and Kakuma, Ryota and Kawana, Kojiro and Kikuta, Satoshi and Kobayashi, Umi and Koike, Michitaro and Komiyama, Yutaka and Li, Xiangchong and Liang, Yongming and Lin, Yen-Ting and Luo, Wentao and Lupton, Robert and Lust, Nate B. and MacArthur, Lauren A. and Matsuoka, Yoshiki and Mineo, Sogo and Miyatake, Hironao and Miyazaki, Satoshi and More, Surhud and Murata, Ryoma and Namiki, Shigeru V. and Nishizawa, Atsushi J. and Oguri, Masamune and Okabe, Nobuhiro and Okamoto, Sakurako and Okura, Yuki and Ono, Yoshiaki and Onodera, Masato and Onoue, Masafusa and Osato, Ken and Ouchi, Masami and Shibuya, Takatoshi and Strauss, Michael A. and Sugiyama, Naoshi and Suto, Yasushi and Takada, Masahiro and Takagi, Yuhei and Takata, Tadafumi and Takita, Satoshi and Tanaka, Masayuki and Terai, Tsuyoshi and Toba, Yoshiki and Uchiyama, Hisakazu and Utsumi, Yousuke and Wang, Shiang-Yu and Wang, Wenting and Yamada, Yoshihiko},
	month = dec,
	year = {2019},
	keywords = {astronomical databases: miscellaneous, cosmology: observations, galaxies: general, surveys},
	pages = {114}
}

@article{mccracken_ultravista_2012,
	title = {{UltraVISTA}: a new ultra-deep near-infrared survey in {COSMOS}},
	volume = {544},
	issn = {0004-6361},
	shorttitle = {{UltraVISTA}},
	url = {http://adsabs.harvard.edu/abs/2012A%26A...544A.156M},
	doi = {10.1051/0004-6361/201219507},
	abstract = {In this paper we describe the first data release of the UltraVISTA near-infrared imaging survey of the COSMOS field. We summarise the key goals and design of the survey and provide a detailed description of our data reduction techniques. We provide stacked, sky-subtracted images in YJHKs and narrow-band filters constructed from data collected during the first year of UltraVISTA observations. Our stacked images reach 5σAB depths in an aperture of 2″ diameter of {\textasciitilde}25 in Y
and {\textasciitilde}24 in JHKs bands and all have sub-arcsecond seeing. To this 5σ limit, our Ks catalogue contains 216 268
sources. We carry out a series of quality assessment tests on our images and catalogues, comparing our stacks with existing catalogues. The 1σ astrometric rms in both directions for stars selected with 17.0 {\textless} Ks(AB) {\textless} 19.5 is {\textasciitilde}0.08″ in comparison to the
publicly-available COSMOS ACS catalogues. Our images are resampled to the same pixel scale and tangent point as the publicly available COSMOS data and so may be easily used to generate multi-colour catalogues using this data. All images and catalogues presented in this paper are publicly available through ESO's "phase 3" archiving and distribution system and from the UltraVISTA web site.

Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under ESO programme ID 179.A-2005 and on data products produced by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium.Catalogs are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/544/A156},
	urldate = {2020-05-08},
	journal = {Astronomy and Astrophysics},
	author = {McCracken, H. J. and Milvang-Jensen, B. and Dunlop, J. and Franx, M. and Fynbo, J. P. U. and Le Fèvre, O. and Holt, J. and Caputi, K. I. and Goranova, Y. and Buitrago, F. and Emerson, J. P. and Freudling, W. and Hudelot, P. and López-Sanjuan, C. and Magnard, F. and Mellier, Y. and Møller, P. and Nilsson, K. K. and Sutherland, W. and Tasca, L. and Zabl, J.},
	month = aug,
	year = {2012},
	keywords = {cosmology: observations, galaxies: general, galaxies: high-redshift, large-scale structure of Universe, surveys},
	pages = {A156}
}

@article{sawicki_cfht_2019,
	title = {The {CFHT} large area {U}-band deep survey ({CLAUDS})},
	volume = {489},
	issn = {0035-8711},
	url = {http://adsabs.harvard.edu/abs/2019MNRAS.489.5202S},
	doi = {10.1093/mnras/stz2522},
	abstract = {The Canada-France-Hawaii Telescope (CFHT) Large Area U-band Deep Survey (CLAUDS) uses data taken with the MegaCam mosaic imager on CFHT to produce images of 18.60 deg{\textasciicircum}2 with median seeing of FWHM = 0.92 arcsec and to a median depth of U = 27.1 AB (5σ in 2 arcsec apertures), with selected areas that total 1.36 deg{\textasciicircum}2 reaching a median depth of U=27.7 AB. These are the deepest U-band images assembled to date over this large an area. These data are located in four fields also imaged to comparably faint levels in grizy and several narrowband filters as part of the Hyper Suprime-Cam (HSC) Subaru Strategic Program (HSC-SSP). These CFHT and Subaru data sets will remain unmatched in their combination of area and depth until the advent of the Large Synoptic Survey Telescope. This paper provides an overview of the scientific motivation for CLAUDS and gives details of the observing strategy, observations, data reduction, and data merging with the HSC-SSP. Three early applications of these deep data are used to illustrate the potential of the data set: deep U-band galaxy number counts, z∼ 3 Lyman break galaxy selection, and photometric redshifts improved by adding CLAUDS U to the Subaru HSC grizy photometry.},
	urldate = {2020-05-08},
	journal = {Monthly Notices of the Royal Astronomical Society},
	author = {Sawicki, Marcin and Arnouts, Stephane and Huang, Jiasheng and Coupon, Jean and Golob, Anneya and Gwyn, Stephen and Foucaud, Sebastien and Moutard, Thibaud and Iwata, Ikuru and Liu, Chengze and Chen, Lingjian and Desprez, Guillaume and Harikane, Yuichi and Ono, Yoshiaki and Strauss, Michael A. and Tanaka, Masayuki and Thibert, Nathalie and Balogh, Michael and Bundy, Kevin and Chapman, Scott and Gunn, James E. and Hsieh, Bau-Ching and Ilbert, Olivier and Jing, Yipeng and LeFèvre, Olivier and Li, Cheng and Matsuda, Yuichi and Miyazaki, Satoshi and Nagao, Tohru and Nishizawa, Atsushi J. and Ouchi, Masami and Shimasaku, Kazuhiro and Silverman, John and de la Torre, Sylvain and Tresse, Laurence and Wang, Wei-Hao and Willott, Chris J. and Yamada, Toru and Yang, Xiaohu and Yee, Howard K. C.},
	month = nov,
	year = {2019},
	keywords = {cosmology: observations, dark matter, galaxies: formation, galaxies: haloes, galaxies: statistics, large-scale structure of universe},
	pages = {5202--5217}
}

@article{taniguchi_subaru_2015,
	title = {The {Subaru} {COSMOS} 20: {Subaru} optical imaging of the {HST} {COSMOS} field with 20 filters*},
	volume = {67},
	issn = {0004-6264},
	shorttitle = {The {Subaru} {COSMOS} 20},
	url = {http://adsabs.harvard.edu/abs/2015PASJ...67..104T},
	doi = {10.1093/pasj/psv106},
	abstract = {We present both the observations and the data reduction procedures of 
the Subaru COSMOS 20 project, an optical imaging survey of the HST
COSMOS field, carried out by using Suprime-Cam on the Subaru Telescope
with the following 20 optical filters: six broad-band (B, g', V, r', i',
and z'), two narrow-band (NB711 and NB816), and 12 intermediate-band
filters (IA427, IA464, IA484, IA505, IA527, IA574, IA624, IA679, IA709,
IA738, IA767, and IA827). Part of this project is described in Taniguchi
et al. (2007, ApJS, 172, 9) and Capak et al. (2007, ApJS, 172, 99) for
the six broad-band and one narrow-band (NB816) filter data. In this
paper, we present details of the observations and data reduction for the
remaining 13 filters (the 12 IA filters and NB711). In particular, we
describe the accuracy of both the photometry and astrometry in all the
filter bands. We also present the optical properties of the Suprime-Cam
IA filter system in appendices.},
	urldate = {2020-05-08},
	journal = {Publications of the Astronomical Society of Japan},
	author = {Taniguchi, Yoshiaki and Kajisawa, Masaru and Kobayashi, Masakazu A. R. and Shioya, Yasuhiro and Nagao, Tohru and Capak, Peter L. and Aussel, Herve and Ichikawa, Akie and Murayama, Takashi and Scoville, Nick Z. and Ilbert, Olivier and Salvato, Mara and Sanders, David B. B. and Mobasher, Bahram and Miyazaki, Satoshi and Komiyama, Yutaka and Le Fèvre, Olivier and Tasca, Lidia and Lilly, Simon and Carollo, Marcella and Renzini, Alvio and Rich, Michael and Schinnerer, Eva and Kaifu, Norio and Karoji, Hiroshi and Arimoto, Nobuo and Okamura, Sadanori and Ohta, Kouji and Shimasaku, Kazuhiro and Hayashino, Tomoki},
	month = dec,
	year = {2015},
	keywords = {methods: observational, surveys, techniques: photometric},
	pages = {104}
}

@article{taniguchi_cosmic_2007,
	title = {The {Cosmic} {Evolution} {Survey} ({COSMOS}): {Subaru} {Observations} of the {HST} {Cosmos} {Field}},
	volume = {172},
	issn = {0067-0049},
	shorttitle = {The {Cosmic} {Evolution} {Survey} ({COSMOS})},
	url = {http://adsabs.harvard.edu/abs/2007ApJS..172....9T},
	doi = {10.1086/516596},
	abstract = {We present deep optical imaging observations of 2 square degree area, 
covered by the Cosmic Evolution Survey (COSMOS), made by the prime-focus
camera (Supreme-Cam) on the 8.2 m Subaru Telescope. Observations were
done in six broadband [B (4459.7 Å), g' (4723.1
Å), V (5483.8 Å), r' (6213.0 Å),
i' (7640.8 Å), z' (8855.0 Å)] and one
narrowband (NB816) filters. A total of 106 galaxies were
detected to i'{\textasciitilde}26.5 mag. These data, combined with
observations at u* and K-band are used to construct the
photometric catalogs for the COSMOS, to measure their photometric
redshifts, multiband spectral energy distributions, and stellar masses,
and to identify high-redshift candidates. This catalog provides
multi-wave band data for scientific analysis of the COSMOS survey.

Based on data collected at Subaru Telescope, which is operated by the
National Astronomical Observatory of Japan.},
	urldate = {2020-05-08},
	journal = {The Astrophysical Journal Supplement Series},
	author = {Taniguchi, Y. and Scoville, N. and Murayama, T. and Sanders, D. B. and Mobasher, B. and Aussel, H. and Capak, P. and Ajiki, M. and Miyazaki, S. and Komiyama, Y. and Shioya, Y. and Nagao, T. and Sasaki, S. S. and Koda, J. and Carilli, C. and Giavalisco, M. and Guzzo, L. and Hasinger, G. and Impey, C. and LeFevre, O. and Lilly, S. and Renzini, A. and Rich, M. and Schinnerer, E. and Shopbell, P. and Kaifu, N. and Karoji, H. and Arimoto, N. and Okamura, S. and Ohta, K.},
	month = sep,
	year = {2007},
	keywords = {Galaxies: Evolution, Galaxies: Interactions},
	pages = {9--28}
}

@article{massey_polar_2005,
	title = {Polar shapelets},
	volume = {363},
	issn = {0035-8711},
	url = {http://adsabs.harvard.edu/abs/2005MNRAS.363..197M},
	doi = {10.1111/j.1365-2966.2005.09453.x},
	abstract = {The shapelets method for image analysis is based upon the decomposition of localized objects into a series of orthogonal components with convenient mathematical properties. We extend the `Cartesian shapelet' formalism from earlier work, and construct `polar shapelet' basis functions that separate an image into components with explicit
rotational symmetries. These frequently provide a more compact
parametrization, and can be interpreted in an intuitive way. Image manipulation in shapelet space is simplified by the concise expressions for linear coordinate transformations, and shape measures (including object photometry, astrometry and galaxy morphology estimators) take a naturally elegant form. Particular attention is paid to the analysis of astronomical survey images, and we test shapelet techniques upon real data from the Hubble Space Telescope. We present a practical method to automatically optimize the quality of an arbitrary shapelet
decomposition in the presence of observational noise, pixelization and a point spread function. A central component of this procedure is the adaptive choice of the scale size and the truncation order of the shapelet expansion. A complete software package to perform shapelet image analysis is made available on the World Wide Web.},
	urldate = {2020-05-08},
	journal = {Monthly Notices of the Royal Astronomical Society},
	author = {Massey, Richard and Refregier, Alexandre},
	month = oct,
	year = {2005},
	keywords = {galaxies: fundamental parameters, methods: analytical, methods: data analysis, techniques: image processing},
	pages = {197--210}
}

@article{moffat_theoretical_1969,
	title = {A {Theoretical} {Investigation} of {Focal} {Stellar} {Images} in the {Photographic} {Emulsion} and {Application} to {Photographic} {Photometry}},
	volume = {3},
	issn = {0004-6361},
	url = {http://adsabs.harvard.edu/abs/1969A%26A.....3..455M},
	abstract = {Two-dimensional intensity proffles of focal stellar images in 
photographic emulsions were derived by convolving gaussian seeing
distributions with diffraction proffles and emulsion scattering
functions. The results predict too low an intensity for large radial
distances from the centre of the image, contradicting the assumption
that seeing is gaussian. An analytic formula representing observed image
proffles combined with an expression for the characteristic curve led to
calibration curves for iris photometers. The curves which were based on
five physical parameters were tested using photoelectric standards and
found to be valid over at least six magnitudes including the plate
limit. These parameters can be determined from bright standard stars
making it possible to obtain magnitudes of faint stars for which there
are no photoelectric standards. In the case of variable background
intensity the theory predicts too small an iris diameter for bright
stars imbedded in bright background. This is due to neglection of the
depth of the emulsion.},
	urldate = {2020-05-08},
	journal = {Astronomy and Astrophysics},
	author = {Moffat, A. F. J.},
	month = dec,
	year = {1969},
	pages = {455}
}

@article{bertin_psfex_2013,
	title = {{PSFEx}: {Point} {Spread} {Function} {Extractor}},
	shorttitle = {{PSFEx}},
	url = {http://adsabs.harvard.edu/abs/2013ascl.soft01001B},
	abstract = {PSFEx (“PSF Extractor”) extracts models of the Point Spread Function (PSF) from FITS images processed with SExtractor and measures the quality of images. The generated PSF models can be used for model-fitting photometry or morphological analyses.},
	urldate = {2020-05-08},
	journal = {Astrophysics Source Code Library},
	author = {Bertin, Emmanuel},
	month = jan,
	year = {2013},
	keywords = {Software},
	pages = {ascl:1301.001}
}

@article{schlegel_maps_1998,
	title = {Maps of {Dust} {Infrared} {Emission} for {Use} in {Estimation} of {Reddening} and {Cosmic} {Microwave} {Background} {Radiation} {Foregrounds}},
	volume = {500},
	issn = {0004-637X},
	url = {http://adsabs.harvard.edu/abs/1998ApJ...500..525S},
	doi = {10.1086/305772},
	abstract = {We present a full-sky 100 μm map that is a reprocessed composite of 
the COBE/DIRBE and IRAS/ISSA maps, with the zodiacal foreground and
confirmed point sources removed. Before using the ISSA maps, we remove
the remaining artifacts from the IRAS scan pattern. Using the DIRBE 100
and 240 μm data, we have constructed a map of the dust temperature so
that the 100 μm map may be converted to a map proportional to dust
column density. The dust temperature varies from 17 to 21 K, which is
modest but does modify the estimate of the dust column by a factor of 5.
The result of these manipulations is a map with DIRBE quality
calibration and IRAS resolution. A wealth of filamentary detail is
apparent on many different scales at all Galactic latitudes. In
high-latitude regions, the dust map correlates well with maps of H I
emission, but deviations are coherent in the sky and are especially
conspicuous in regions of saturation of H I emission toward denser
clouds and of formation of H2 in molecular clouds. In
contrast, high-velocity H I clouds are deficient in dust emission, as
expected.

To generate the full-sky dust maps, we must first remove zodiacal light
contamination, as well as a possible cosmic infrared background (CIB).
This is done via a regression analysis of the 100 μm DIRBE map
against the Leiden-Dwingeloo map of H I emission, with corrections for
the zodiacal light via a suitable expansion of the DIRBE 25 μm flux.
This procedure removes virtually all traces of the zodiacal foreground.
For the 100 μm map no significant CIB is detected. At longer
wavelengths, where the zodiacal contamination is weaker, we detect the
CIB at surprisingly high flux levels of 32 +/- 13 nW m-2
sr-1 at 140 μm and of 17 +/- 4 nW m-2
sr-1 at 240 μm (95\% confidence). This integrated flux {\textasciitilde}2
times that extrapolated from optical galaxies in the Hubble Deep Field.

The primary use of these maps is likely to be as a new estimator of
Galactic extinction. To calibrate our maps, we assume a standard
reddening law and use the colors of elliptical galaxies to measure the
reddening per unit flux density of 100 μm emission. We find
consistent calibration using the B-R color distribution of a sample of
the 106 brightest cluster ellipticals, as well as a sample of 384
ellipticals with B-V and Mg line strength measurements. For the latter
sample, we use the correlation of intrinsic B-V versus Mg2
index to tighten the power of the test greatly. We demonstrate that the
new maps are twice as accurate as the older Burstein-Heiles reddening
estimates in regions of low and moderate reddening. The maps are
expected to be significantly more accurate in regions of high reddening.
These dust maps will also be useful for estimating millimeter emission
that contaminates cosmic microwave background radiation experiments and
for estimating soft X-ray absorption. We describe how to access our maps
readily for general use.},
	urldate = {2020-05-08},
	journal = {The Astrophysical Journal},
	author = {Schlegel, David J. and Finkbeiner, Douglas P. and Davis, Marc},
	month = jun,
	year = {1998},
	keywords = {Cosmology: Cosmic Microwave Background, COSMOLOGY: COSMIC MICROWAVE BACKGROUND, Cosmology: Diffuse Radiation, COSMOLOGY: DIFFUSE RADIATION, Extinction, EXTINCTION, Infrared: ISM: Continuum, INFRARED: ISM: CONTINUUM, Interplanetary Medium, INTERPLANETARY MEDIUM, ISM: Dust, ISM: DUST},
	pages = {525--553}
}

@article{schlafly_measuring_2011,
	title = {Measuring {Reddening} with {Sloan} {Digital} {Sky} {Survey} {Stellar} {Spectra} and {Recalibrating} {SFD}},
	volume = {737},
	issn = {0004-637X},
	url = {http://adsabs.harvard.edu/abs/2011ApJ...737..103S},
	doi = {10.1088/0004-637X/737/2/103},
	abstract = {We present measurements of dust reddening using the colors of stars with 
spectra in the Sloan Digital Sky Survey. We measure reddening as the
difference between the measured and predicted colors of a star, as
derived from stellar parameters from the Sloan Extension for Galactic
Understanding and Exploration Stellar Parameter Pipeline. We achieve
uncertainties of 56, 34, 25, and 29 mmag in the colors u - g, g - r, r -
i, and i - z, per star, though the uncertainty varies depending on the
stellar type and the magnitude of the star. The spectrum-based reddening
measurements confirm our earlier "blue tip" reddening measurements,
finding reddening coefficients different by -3\%, 1\%, 1\%, and 2\% in u -
g, g - r, r - i, and i - z from those found by the blue tip method,
after removing a 4\% normalization difference. These results prefer an
RV = 3.1 Fitzpatrick reddening law to O'Donnell or Cardelli
et al. reddening laws. We provide a table of conversion coefficients
from the Schlegel et al. (SFD) maps of E(B - V) to extinction in 88
bandpasses for four values of RV , using this reddening law
and the 14\% recalibration of SFD first reported by Schlafly et al. and
confirmed in this work.},
	urldate = {2020-05-08},
	journal = {The Astrophysical Journal},
	author = {Schlafly, Edward F. and Finkbeiner, Douglas P.},
	month = aug,
	year = {2011},
	keywords = {dust, extinction, Galaxy: stellar content, ISM: clouds},
	pages = {103}
}

@article{capak_first_2007,
	title = {The {First} {Release} {COSMOS} {Optical} and {Near}-{IR} {Data} and {Catalog}},
	volume = {172},
	issn = {0067-0049},
	url = {http://adsabs.harvard.edu/abs/2007ApJS..172...99C},
	doi = {10.1086/519081},
	abstract = {We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3 and 2.4 μm. These include data taken on the Subaru 8.3 m telescope, the KPNO and CTIO 4 m telescopes, and the CFHT 3.6 m telescope. Special techniques are used to ensure that the relative photometric calibration is better than 1\% across the field of view. The absolute photometric accuracy from standard-star measurements is found to be 6\%. The absolute calibration is corrected using galaxy spectra, providing colors accurate to 2\% or better. Stellar and galaxy colors and counts agree well with the expected values. Finally, as the first step in the scientific analysis of these data we construct panchromatic number counts which confirm that both the geometry of the universe and the galaxy population are evolving.

Based in part on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS5-26555 the Subaru telescope, which is operated by the National Astronomical Observatory of Japan; the MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA at the Canada-France-Hawaii Telescope, which is operated by the National Research Council of Canada, the Institute National des Science de l'Univers of the Centre National de la Recherche, and the University of Hawaii; and the Kitt Peak National Observatory, Cerro Tololo
Inter-American Observatory, and the National Optical Astronomy
Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation.},
	urldate = {2020-05-08},
	journal = {The Astrophysical Journal Supplement Series},
	author = {Capak, P. and Aussel, H. and Ajiki, M. and McCracken, H. J. and Mobasher, B. and Scoville, N. and Shopbell, P. and Taniguchi, Y. and Thompson, D. and Tribiano, S. and Sasaki, S. and Blain, A. W. and Brusa, M. and Carilli, C. and Comastri, A. and Carollo, C. M. and Cassata, P. and Colbert, J. and Ellis, R. S. and Elvis, M. and Giavalisco, M. and Green, W. and Guzzo, L. and Hasinger, G. and Ilbert, O. and Impey, C. and Jahnke, K. and Kartaltepe, J. and Kneib, J.-P. and Koda, J. and Koekemoer, A. and Komiyama, Y. and Leauthaud, A. and Le Fevre, O. and Lilly, S. and Liu, C. and Massey, R. and Miyazaki, S. and Murayama, T. and Nagao, T. and Peacock, J. A. and Pickles, A. and Porciani, C. and Renzini, A. and Rhodes, J. and Rich, M. and Salvato, M. and Sanders, D. B. and Scarlata, C. and Schiminovich, D. and Schinnerer, E. and Scodeggio, M. and Sheth, K. and Shioya, Y. and Tasca, L. A. M. and Taylor, J. E. and Yan, L. and Zamorani, G.},
	month = sep,
	year = {2007},
	keywords = {Cosmology: Large-Scale Structure of Universe, Cosmology: Observations, Galaxies: Evolution, Surveys},
	pages = {99--116}
}

@article{mccracken_cosmos-wircam_2010,
	title = {The {COSMOS}-{WIRCam} {Near}-{Infrared} {Imaging} {Survey}. {I}. {BzK}-{Selected} {Passive} and {Star}-{Forming} {Galaxy} {Candidates} at z gsim 1.4},
	volume = {708},
	issn = {0004-637X},
	url = {http://adsabs.harvard.edu/abs/2010ApJ...708..202M},
	doi = {10.1088/0004-637X/708/1/202},
	abstract = {We present a new near-infrared survey covering the 2 deg2 
COSMOS field conducted using WIRCam at the Canada-France-Hawaii
Telescope. By combining our near-infrared data with Subaru B and z
images, we construct a deep, wide-field optical-infrared catalog. At K
s {\textless} 23 (AB magnitudes), our survey completeness is greater
than 90\% and 70\% for stars and galaxies, respectively, and contains
143,466 galaxies and 13,254 stars. Using the BzK diagram, we divide our
galaxy catalog into quiescent and star-forming galaxy candidates. At z {\textasciitilde}
2, our catalogs contain 3931 quiescent and 25,757 star-forming galaxies
representing the largest and most secure sample at these depths and
redshifts to date. Our counts of quiescent galaxies turns over at K
s {\textasciitilde} 22, an effect that we demonstrate cannot be due to sample
incompleteness. Both the number of faint and bright quiescent objects in
our catalogs exceed the predictions of a recent semi-analytic model of
galaxy formation, indicating potentially the need for further
refinements in the amount of merging and active galactic nucleus
feedback at z {\textasciitilde} 2 in these models. We measure the angular correlation
function for each sample and find that the slope of the field galaxy
correlation function flattens to 1.5 by K s {\textasciitilde} 23. At small
angular scales, the angular correlation function for passive BzK
galaxies is considerably in excess of the clustering of dark matter. We
use precise 30-band photometric redshifts to derive the spatial
correlation length and the redshift distributions for each object class.
At K s {\textless} 22, we find r γ/1.8 0
= 7.0 ± 0.5h -1 Mpc for the passive BzK candidates and
4.7 ± 0.8 h -1 Mpc for the star-forming BzK galaxies.
Our pBzK galaxies have an average photometric redshift of zp
{\textasciitilde} 1.4, in approximate agreement with the limited spectroscopic
information currently available. The stacked K s image will
be made publicly available from IRSA.

Based on data collected at the Subaru Telescope, which is operated by
the National Astronomical Observatory of Japan; the European Southern
Observatory under Large Program 175.A-0839, Chile and the
Canada-France-Hawaii Telescope with WIRCam and MegaPrime/MegaCam, the
latter operated as a joint project by the CFHT Corporation, CEA/DAPNIA,
the NRC and CADC of Canada, the CNRS of France, TERAPIX, and the
University of Hawaii. This research has made use of the NASA/IPAC
Infrared Science Archive, which is operated by the Jet Propulsion
Laboratory (JPL), California Institute of Technology, under contract
with the National Aeronautics and Space Administration. Support for this
work was provided by the Spitzer Science Center, which is operated by
the JPL, California Institute of Technology under NASA contract 1407,
NASA through contract 1278386 issued by the JPL.},
	urldate = {2020-05-08},
	journal = {The Astrophysical Journal},
	author = {McCracken, H. J. and Capak, P. and Salvato, M. and Aussel, H. and Thompson, D. and Daddi, E. and Sanders, D. B. and Kneib, J.-P. and Willott, C. J. and Mancini, C. and Renzini, A. and Cook, R. and Le Fèvre, O. and Ilbert, O. and Kartaltepe, J. and Koekemoer, A. M. and Mellier, Y. and Murayama, T. and Scoville, N. Z. and Shioya, Y. and Tanaguchi, Y.},
	month = jan,
	year = {2010},
	keywords = {cosmology: observations, dark matter, galaxies: evolution, galaxies: formation, large-scale structure of universe, surveys},
	pages = {202--217}
}

@article{ilbert_mass_2013,
	title = {Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from {UltraVISTA}},
	volume = {556},
	issn = {0004-6361},
	url = {http://adsabs.harvard.edu/abs/2013A%26A...556A..55I},
	doi = {10.1051/0004-6361/201321100},
	abstract = {We estimate the galaxy stellar mass function and stellar mass density 
for star-forming and quiescent galaxies with 0.2 {\textless} z {\textless} 4. We
construct a large, deep (Ks {\textless} 24) sample of 220 000
galaxies selected using the new UltraVISTA DR1 data release. Our
analysis is based on precise 30-band photometricredshifts. By comparing
these photometric redshifts with 10,800 spectroscopic redshifts from the
zCOSMOS bright and faint surveys, we find a precision of
σΔz/(1 + z) = 0.008 at i+ {\textless} 22.5
and σΔz/(1 + z) = 0.03 at 1.5 {\textless} z {\textless} 4. We
derive the stellar mass function and correct for the Eddington bias. We
find a mass-dependent evolution of the global and star-forming
populations, with the low-mass end of the mass functions evolving more
rapidly than the high-mass end. This mass-dependent evolution is a
direct consequence of the star formation being "quenched" in galaxies
more massive than ℳ ≳ 1010.7 -
10.9ℳ⊙. For the mass function of the
quiescent galaxies, we do not find any significant evolution of the
high-mass end at z {\textless} 1; however we observe a clear flattening of the
faint-end slope. From z {\textasciitilde} 3 to z {\textasciitilde} 1, the density of quiescent galaxies
increases over the entire mass range. Their comoving stellar mass
density increases by 1.6 dex between z {\textasciitilde} 3 and z {\textasciitilde} 1 and by less than
0.2 dex at z {\textless} 1. We infer the star formation history from the mass
density evolution. This inferred star formation history is in excellent
agreement with instantaneous star formation rate measurements at z {\textless}
1.5, while we find differences of 0.2 dex at z {\textgreater} 1.5 consistent with
the expected uncertainties. We also develop a new method to infer the
specific star formation rate from the mass function of star-forming
galaxies. We find that the specific star formation rate of 1010 -
10.5ℳ⊙ galaxies increases continuously in
the redshift range 1 {\textless} z {\textless} 4. Finally, we compare our results with
a semi-analytical model and find that these models overestimate the
density of low mass quiescent galaxies by an order of magnitude, while
the density of low-mass star-forming galaxies is successfully
reproduced.

Based on data products from observations made with ESO Telescopes at the
La Silla Paranal Observatory under ESO programme ID 179.A-2005 and on
data products produced by TERAPIX and the Cambridge Astronomy Survey
Unit on behalf of the UltraVISTA consortium.Catalogues are only
available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr
(ftp://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/556/A55},
	urldate = {2020-05-08},
	journal = {Astronomy and Astrophysics},
	author = {Ilbert, O. and McCracken, H. J. and Le Fèvre, O. and Capak, P. and Dunlop, J. and Karim, A. and Renzini, M. A. and Caputi, K. and Boissier, S. and Arnouts, S. and Aussel, H. and Comparat, J. and Guo, Q. and Hudelot, P. and Kartaltepe, J. and Kneib, J. P. and Krogager, J. K. and Le Floc'h, E. and Lilly, S. and Mellier, Y. and Milvang-Jensen, B. and Moutard, T. and Onodera, M. and Richard, J. and Salvato, M. and Sanders, D. B. and Scoville, N. and Silverman, J. D. and Taniguchi, Y. and Tasca, L. and Thomas, R. and Toft, S. and Tresse, L. and Vergani, D. and Wolk, M. and Zirm, A.},
	month = aug,
	year = {2013},
	keywords = {galaxies: distances and redshifts, galaxies: evolution, galaxies: formation, galaxies: star formation, galaxies: stellar content},
	pages = {A55}
}

@article{muzzin_public_2013,
	title = {A {Public} {Ks} -selected {Catalog} in the {COSMOS}/{ULTRAVISTA} {Field}: {Photometry}, {Photometric} {Redshifts}, and {Stellar} {Population} {Parameters}},
	volume = {206},
	issn = {0067-0049},
	shorttitle = {A {Public} {Ks} -selected {Catalog} in the {COSMOS}/{ULTRAVISTA} {Field}},
	url = {http://adsabs.harvard.edu/abs/2013ApJS..206....8M},
	doi = {10.1088/0067-0049/206/1/8},
	abstract = {We present a catalog covering 1.62 deg2 of the 
COSMOS/UltraVISTA field with point-spread function (PSF) matched
photometry in 30 photometric bands. The catalog covers the wavelength
range 0.15-24 μm including the available GALEX, Subaru,
Canada-France-Hawaii Telescope, VISTA, and Spitzer data. Catalog sources
have been selected from the DR1 UltraVISTA Ks band imaging
that reaches a depth of K s, tot = 23.4 AB (90\%
completeness). The PSF-matched catalog is generated using
position-dependent PSFs ensuring accurate colors across the entire
field. Also included is a catalog of photometric redshifts (z
phot) for all galaxies computed with the EAZY code.
Comparison with spectroscopy from the zCOSMOS 10k bright sample shows
that up to z {\textasciitilde} 1.5 the z phot are accurate to Δz/(1 +
z) = 0.013, with a catastrophic outlier fraction of only 1.6\%. The z
phot also show good agreement with the z phot from
the NEWFIRM Medium Band Survey out to z {\textasciitilde} 3. A catalog of stellar masses
and stellar population parameters for galaxies determined using the FAST
spectral energy distribution fitting code is provided for all galaxies.
Also included are rest-frame U - V and V - J colors, L
2800 and L IR. The UVJ color-color diagram
confirms that the galaxy bi-modality is well-established out to z {\textasciitilde} 2.
Star-forming galaxies also obey a star-forming "main sequence" out to z
{\textasciitilde} 2.5, and this sequence evolves in a manner consistent with previous
measurements. The COSMOS/UltraVISTA Ks -selected catalog
covers a unique parameter space in both depth, area, and
multi-wavelength coverage and promises to be a useful tool for studying
the growth of the galaxy population out to z {\textasciitilde} 3-4.

.},
	urldate = {2020-05-08},
	journal = {The Astrophysical Journal Supplement Series},
	author = {Muzzin, Adam and Marchesini, Danilo and Stefanon, Mauro and Franx, Marijn and Milvang-Jensen, Bo and Dunlop, James S. and Fynbo, J. P. U. and Brammer, Gabriel and Labbé, Ivo and van Dokkum, Pieter},
	month = may,
	year = {2013},
	keywords = {galaxies: evolution, galaxies: fundamental parameters, galaxies: high-redshift, infrared: galaxies},
	pages = {8}
}

@article{civano_chandra_2016,
	title = {The {Chandra} {Cosmos} {Legacy} {Survey}: {Overview} and {Point} {Source} {Catalog}},
	volume = {819},
	issn = {0004-637X},
	shorttitle = {The {Chandra} {Cosmos} {Legacy} {Survey}},
	url = {http://adsabs.harvard.edu/abs/2016ApJ...819...62C},
	doi = {10.3847/0004-637X/819/1/62},
	abstract = {The COSMOS-Legacy survey is a 4.6 Ms Chandra program that has imaged 2.2 deg2 of the COSMOS field with an effective exposure of ≃ 160 ks over the central 1.5 deg2 and of ≃ 80 ks in the remaining area. The survey is the combination of 56 new observations obtained as an X-ray Visionary Project with the previous C-COSMOS survey. We describe the reduction and analysis of the new observations and the properties of 2273 point sources detected above a spurious probability of 2 × 10-5. We also present the updated
properties of the C-COSMOS sources detected in the new data. The whole survey includes 4016 point sources (3814, 2920 and 2440 in the full, soft, and hard band). The limiting depths are 2.2 ×
10-16, 1.5 × 10-15, and 8.9 ×
10-16 \{{\textbackslash}text\{erg cm\}\}-2 \{\{\{s\}\}\}-1 in the 0.5-2, 2-10, and 0.5-10 keV bands, respectively. The observed fraction of obscured active galactic nuclei with a column density {\textgreater}1022 cm-2 from the hardness ratio (HR) is ∼50\{\}-16+17\%. Given the large sample we
compute source number counts in the hard and soft bands, significantly reducing the uncertainties of 5\%-10\%. For the first time we compute number counts for obscured (HR {\textgreater} -0.2) and unobscured (HR {\textless} -0.2) sources and find significant differences between the two populations in the soft band. Due to the unprecedent large exposure, COSMOS-Legacy area is three times larger than surveys at similar depths and its depth is three times fainter than surveys covering similar areas. The area-flux region occupied by COSMOS-Legacy is likely to remain unsurpassed for years to come.},
	urldate = {2020-05-08},
	journal = {The Astrophysical Journal},
	author = {Civano, F. and Marchesi, S. and Comastri, A. and Urry, M. C. and Elvis, M. and Cappelluti, N. and Puccetti, S. and Brusa, M. and Zamorani, G. and Hasinger, G. and Aldcroft, T. and Alexander, D. M. and Allevato, V. and Brunner, H. and Capak, P. and Finoguenov, A. and Fiore, F. and Fruscione, A. and Gilli, R. and Glotfelty, K. and Griffiths, R. E. and Hao, H. and Harrison, F. A. and Jahnke, K. and Kartaltepe, J. and Karim, A. and LaMassa, S. M. and Lanzuisi, G. and Miyaji, T. and Ranalli, P. and Salvato, M. and Sargent, M. and Scoville, N. J. and Schawinski, K. and Schinnerer, E. and Silverman, J. and Smolcic, V. and Stern, D. and Toft, S. and Trakhtenbrot, B. and Treister, E. and Vignali, C.},
	month = mar,
	year = {2016},
	keywords = {catalogs, cosmology: observations, galaxies: evolution, quasars: general, surveys, X-rays: general},
	pages = {62}
}

@article{marchesi_chandra_2016,
	title = {The {Chandra} {COSMOS} {Legacy} survey: optical/{IR} identifications},
	volume = {817},
	issn = {0004-637X},
	shorttitle = {The {Chandra} {COSMOS} {Legacy} survey},
	url = {http://adsabs.harvard.edu/abs/2016ApJ...817...34M},
	doi = {10.3847/0004-637X/817/1/34},
	abstract = {We present the catalog of optical and infrared counterparts of the Chandra COSMOS-Legacy Survey, a 4.6 Ms Chandra program on the 2.2 deg2 of the COSMOS field, combination of 56 new overlapping observations obtained in Cycle 14 with the previous C-COSMOS survey. In this Paper we report the I, K, and 3.6 μm identifications of the 2273 X-ray point sources detected in the new Cycle 14 observations. We use the likelihood ratio technique to derive the association of
optical/infrared (IR) counterparts for 97\% of the X-ray sources. We also update the information for the 1743 sources detected in C-COSMOS, using new K and 3.6 μm information not available when the C-COSMOS analysis was performed. The final catalog contains 4016 X-ray sources, 97\% of which have an optical/IR counterpart and a photometric redshift, while ≃54\% of the sources have a spectroscopic redshift. The full
catalog, including spectroscopic and photometric redshifts and optical and X-ray properties described here in detail, is available online. We study several X-ray to optical (X/O) properties: with our large
statistics we put better constraints on the X/O flux ratio locus, finding a shift toward faint optical magnitudes in both soft and hard X-ray band. We confirm the existence of a correlation between X/O and the the 2-10 keV luminosity for Type 2 sources. We extend to low luminosities the analysis of the correlation between the fraction of obscured AGNs and the hard band luminosity, finding a different behavior between the optically and X-ray classified obscured fraction.},
	urldate = {2020-05-08},
	journal = {The Astrophysical Journal},
	author = {Marchesi, S. and Civano, F. and Elvis, M. and Salvato, M. and Brusa, M. and Comastri, A. and Gilli, R. and Hasinger, G. and Lanzuisi, G. and Miyaji, T. and Treister, E. and Urry, C. M. and Vignali, C. and Zamorani, G. and Allevato, V. and Cappelluti, N. and Cardamone, C. and Finoguenov, A. and Griffiths, R. E. and Karim, A. and Laigle, C. and LaMassa, S. M. and Jahnke, K. and Ranalli, P. and Schawinski, K. and Schinnerer, E. and Silverman, J. D. and Smolcic, V. and Suh, H. and Trakhtenbrot, B.},
	month = jan,
	year = {2016},
	keywords = {catalogs, cosmology: observations, galaxies: active, galaxies: evolution, surveys, X-rays: general},
	pages = {34}
}

@article{jin_super-deblended_2018,
	title = {“{Super}-deblended” {Dust} {Emission} in {Galaxies}. {II}. {Far}-{IR} to ({Sub})millimeter {Photometry} and {High}-redshift {Galaxy} {Candidates} in the {Full} {COSMOS} {Field}},
	volume = {864},
	issn = {0004-637X},
	url = {http://adsabs.harvard.edu/abs/2018ApJ...864...56J},
	doi = {10.3847/1538-4357/aad4af},
	abstract = {We present a “super-deblended” far-infrared (FIR) to 
(sub)millimeter photometric catalog in the Cosmic Evolution Survey
(COSMOS), prepared with the method recently developed by Liu et al.,
with key adaptations. We obtain point-spread function fitting photometry
at fixed prior positions including 88,008 galaxies detected in VLA 1.4,
3 GHz, and/or MIPS 24 μm images. By adding a specifically carved
mass-selected sample (with an evolving stellar mass limit), a highly
complete prior sample of 194,428 galaxies is achieved for deblending
FIR/(sub)mm images. We performed “active” removal of
nonrelevant priors at FIR/(sub)mm bands using spectral energy
distribution fitting and redshift information. In order to cope with the
shallower COSMOS data, we subtract from the maps the flux of faint
nonfitted priors and explicitly account for the uncertainty of this
step. The resulting photometry (including data from Spitzer, Herschel,
SCUBA2, AzTEC, MAMBO, and NSF’s Karl G. Jansky Very Large Array at
3 and 1.4 GHz) displays well-behaved quasi-Gaussian uncertainties
calibrated from Monte Carlo simulations and tailored to observables
(crowding, residual maps). Comparison to ALMA photometry for hundreds of
sources provides a remarkable validation of the technique. We detect
11,220 galaxies over the 100-1200 μm range extending to z
phot ∼ 7. We conservatively selected a sample of 85 z
{\textgreater} 4 high-redshift candidates significantly detected in the
FIR/(sub)mm, often with secure radio and/or Spitzer/IRAC counterparts.
This provides a chance to investigate the first generation of vigorous
starburst galaxies (SFRs ∼ 1000 M ⊙ yr-1).
The photometric and value-added catalogs are publicly released.},
	urldate = {2020-05-08},
	journal = {The Astrophysical Journal},
	author = {Jin, Shuowen and Daddi, Emanuele and Liu, Daizhong and Smolčić, Vernesa and Schinnerer, Eva and Calabrò, Antonello and Gu, Qiusheng and Delhaize, Jacinta and Delvecchio, Ivan and Gao, Yu and Salvato, Mara and Puglisi, Annagrazia and Dickinson, Mark and Bertoldi, Frank and Sargent, Mark and Novak, Mladen and Magdis, Georgios and Aretxaga, Itziar and Wilson, Grant W. and Capak, Peter},
	month = sep,
	year = {2018},
	keywords = {galaxies: ISM, galaxies: photometry, galaxies: star formation, infrared: galaxies, techniques: photometric},
	pages = {56}
}

@article{barbary_sep_2016,
	title = {{SEP}: {Source} {Extractor} as a library},
	volume = {1},
	issn = {2475-9066},
	shorttitle = {{SEP}},
	url = {http://joss.theoj.org/papers/10.21105/joss.00058},
	doi = {10.21105/joss.00058},
	language = {en},
	number = {6},
	urldate = {2020-06-29},
	journal = {The Journal of Open Source Software},
	author = {Barbary, Kyle},
	month = oct,
	year = {2016},
	pages = {58}
}

@article{lang_tractor_2016,
	title = {The {Tractor}: {Probabilistic} astronomical source detection and measurement},
	shorttitle = {The {Tractor}},
	url = {http://adsabs.harvard.edu/abs/2016ascl.soft04008L},
	abstract = {The Tractor optimizes or samples from models of astronomical objects. The approach is generative: given astronomical sources and a description of the image properties, the code produces pixel-space estimates or predictions of what will be observed in the images. This estimate can be used to produce a likelihood for the observed data given the model: assuming the model space actually includes the truth (it doesn’t, in detail), then if we had the optimal model parameters, the predicted image would differ from the actually observed image only by noise. Given a noise model of the instrument and assuming pixelwise independent noise, the log-likelihood is the negative chi-squared difference: (image - model) / noise.},
	urldate = {2020-06-29},
	journal = {Astrophysics Source Code Library},
	author = {Lang, Dustin and Hogg, David W. and Mykytyn, David},
	month = apr,
	year = {2016},
	keywords = {Software},
	pages = {ascl:1604.008}
}

@article{ashby_spitzer_2018,
	title = {Spitzer {Matching} {Survey} of the {UltraVISTA} {Ultra}-deep {Stripes} ({SMUVS}): {Full}-mission {IRAC} {Mosaics} and {Catalogs}},
	volume = {237},
	issn = {0067-0049},
	shorttitle = {Spitzer {Matching} {Survey} of the {UltraVISTA} {Ultra}-deep {Stripes} ({SMUVS})},
	url = {http://adsabs.harvard.edu/abs/2018ApJS..237...39A},
	doi = {10.3847/1538-4365/aad4fb},
	abstract = {This paper describes new deep 3.6 and 4.5 μm imaging of three 
UltraVISTA near-infrared survey stripes within the COSMOS field. The
observations were carried out with Spitzer’s Infrared Array Camera
(IRAC) for the Spitzer Matching Survey of the UltraVISTA Deep Stripes
(SMUVS). In this work we present our data reduction techniques, and
document the resulting mosaics, coverage maps, and catalogs in both IRAC
passbands for the three easternmost UltraVISTA survey stripes, covering
a combined area of about 0.66 deg2, of which 0.45
deg2 have at least 20 hr of integration time. SMUVS reaches
point-source sensitivities of about 25.0 AB mag (0.13 μJy) at both
3.6 and 4.5 μm, with a significance of 4σ, accounting for both
survey sensitivity and source confusion. To this limit the SMUVS
catalogs contain a total of ∼350,000 sources, each of which is
detected significantly in at least one IRAC band. Because of its uniform
and high sensitivity, relatively large area coverage, and the wide array
of ancillary data available in COSMOS, the SMUVS survey will be useful
for a large number of cosmological investigations. We make all images
and catalogs described herein publicly available via the Spitzer Science
Center.},
	urldate = {2020-06-29},
	journal = {The Astrophysical Journal Supplement Series},
	author = {Ashby, M. L. N. and Caputi, Karina I. and Cowley, Will and Deshmukh, Smaran and Dunlop, James S. and Milvang-Jensen, Bo and Fynbo, Johan P. U. and Muzzin, Adam and McCracken, H. J. and Le Fèvre, Olivier and Huang, Jia-Sheng and Zhang, J.},
	month = aug,
	year = {2018},
	keywords = {catalogs, infrared: galaxies, surveys},
	pages = {39}
}

@ARTICLE{leja_uvj_2019,
       author = {{Leja}, Joel and {Tacchella}, Sandro and {Conroy}, Charlie},
        title = "{Beyond UVJ: More Efficient Selection of Quiescent Galaxies with Ultraviolet/Mid-infrared Fluxes}",
      journal = {\apjl},
     keywords = {galaxies: high-redshift, galaxies: star formation, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = jul,
       volume = {880},
       number = {1},
          eid = {L9},
        pages = {L9},
          doi = {10.3847/2041-8213/ab2f8c},
archivePrefix = {arXiv},
       eprint = {1907.02970},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...880L...9L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@article{steinhardt_star_2014,
	title = {Star {Formation} at 4 {\textless} z {\textless} 6 from the {Spitzer} {Large} {Area} {Survey} with {Hyper}-{Suprime}-{Cam} ({SPLASH})},
	volume = {791},
	issn = {0004-637X},
	url = {http://adsabs.harvard.edu/abs/2014ApJ...791L..25S},
	doi = {10.1088/2041-8205/791/2/L25},
	abstract = {Using the first 50\% of data collected for the Spitzer Large Area Survey 
with Hyper-Suprime-Cam observations on the 1.8 deg2
Cosmological Evolution Survey we estimate the masses and star formation
rates of 3398 M * {\textgreater} 1010 M ⊙
star-forming galaxies at 4 {\textless} z {\textless} 6 with a substantial population
up to M * {\textgreater}{\textasciitilde} 1011.5 M ⊙. We
find that the strong correlation between stellar mass and star formation
rate seen at lower redshift (the "main sequence" of star-forming
galaxies) extends to z {\textasciitilde} 6. The observed relation and scatter is
consistent with a continued increase in star formation rate at fixed
mass in line with extrapolations from lower-redshift observations. It is
difficult to explain this continued correlation, especially for the most
massive systems, unless the most massive galaxies are forming stars near
their Eddington-limited rate from their first collapse. Furthermore, we
find no evidence for moderate quenching at higher masses, indicating
quenching either has not occurred prior to z {\textasciitilde} 6 or else occurs rapidly,
so that few galaxies are visible in transition between star-forming and
quenched.},
	urldate = {2020-06-29},
	journal = {The Astrophysical Journal Letters},
	author = {Steinhardt, Charles L. and Speagle, Josh S. and Capak, Peter and Silverman, John D. and Carollo, Marcella and Dunlop, James and Hashimoto, Yasuhiro and Hsieh, Bau-Ching and Ilbert, Olivier and Le Fevre, Olivier and Le Floc'h, Emeric and Lee, Nicholas and Lin, Lihwai and Lin, Yen-Ting and Masters, Dan and McCracken, Henry J. and Nagao, Tohru and Petric, Andreea and Salvato, Mara and Sanders, Dave and Scoville, Nick and Sheth, Kartik and Strauss, Michael A. and Taniguchi, Yoshiaki},
	month = aug,
	year = {2014},
	keywords = {galaxies: evolution},
	pages = {L25}
}

@article{ashby_seds_2013,
	title = {{SEDS}: {The} {Spitzer} {Extended} {Deep} {Survey}. {Survey} {Design}, {Photometry}, and {Deep} {IRAC} {Source} {Counts}},
	volume = {769},
	issn = {0004-637X},
	shorttitle = {{SEDS}},
	url = {http://adsabs.harvard.edu/abs/2013ApJ...769...80A},
	doi = {10.1088/0004-637X/769/1/80},
	abstract = {The Spitzer Extended Deep Survey (SEDS) is a very deep infrared survey 
within five well-known extragalactic science fields: the UKIDSS
Ultra-Deep Survey, the Extended Chandra Deep Field South, COSMOS, the
Hubble Deep Field North, and the Extended Groth Strip. SEDS covers a
total area of 1.46 deg2 to a depth of 26 AB mag (3σ) in
both of the warm Infrared Array Camera (IRAC) bands at 3.6 and 4.5
μm. Because of its uniform depth of coverage in so many
widely-separated fields, SEDS is subject to roughly 25\% smaller errors
due to cosmic variance than a single-field survey of the same size. SEDS
was designed to detect and characterize galaxies from intermediate to
high redshifts (z = 2-7) with a built-in means of assessing the impact
of cosmic variance on the individual fields. Because the full SEDS depth
was accumulated in at least three separate visits to each field,
typically with six-month intervals between visits, SEDS also furnishes
an opportunity to assess the infrared variability of faint objects. This
paper describes the SEDS survey design, processing, and
publicly-available data products. Deep IRAC counts for the more than
300,000 galaxies detected by SEDS are consistent with models based on
known galaxy populations. Discrete IRAC sources contribute 5.6 ±
1.0 and 4.4 ± 0.8 nW m-2 sr-1
at 3.6 and 4.5 μm to the diffuse cosmic infrared background (CIB).
IRAC sources cannot contribute more than half of the total CIB flux
estimated from DIRBE data. Barring an unexpected error in the DIRBE flux
estimates, half the CIB flux must therefore come from a diffuse
component.},
	urldate = {2020-06-29},
	journal = {The Astrophysical Journal},
	author = {Ashby, M. L. N. and Willner, S. P. and Fazio, G. G. and Huang, J.-S. and Arendt, R. and Barmby, P. and Barro, G. and Bell, E. F. and Bouwens, R. and Cattaneo, A. and Croton, D. and Davé, R. and Dunlop, J. S. and Egami, E. and Faber, S. and Finlator, K. and Grogin, N. A. and Guhathakurta, P. and Hernquist, L. and Hora, J. L. and Illingworth, G. and Kashlinsky, A. and Koekemoer, A. M. and Koo, D. C. and Labbé, I. and Li, Y. and Lin, L. and Moseley, H. and Nandra, K. and Newman, J. and Noeske, K. and Ouchi, M. and Peth, M. and Rigopoulou, D. and Robertson, B. and Sarajedini, V. and Simard, L. and Smith, H. A. and Wang, Z. and Wechsler, R. and Weiner, B. and Wilson, G. and Wuyts, S. and Yamada, T. and Yan, H.},
	month = may,
	year = {2013},
	keywords = {galaxies: high-redshift, infrared: galaxies, surveys},
	pages = {80}
}

@article{ashby_s-candels_2015,
	title = {S-{CANDELS}: {The} {Spitzer}-{Cosmic} {Assembly} {Near}-{Infrared} {Deep} {Extragalactic} {Survey}. {Survey} {Design}, {Photometry}, and {Deep} {IRAC} {Source} {Counts}},
	volume = {218},
	issn = {0067-0049},
	shorttitle = {S-{CANDELS}},
	url = {http://adsabs.harvard.edu/abs/2015ApJS..218...33A},
	doi = {10.1088/0067-0049/218/2/33},
	abstract = {The Spitzer-Cosmic Assembly Deep Near-infrared Extragalactic Legacy 
Survey (S-CANDELS; PI G.Fazio) is a Cycle 8 Exploration Program designed
to detect galaxies at very high redshifts (z{\textbackslash}gt 5). To mitigate the
effects of cosmic variance and also to take advantage of deep
coextensive coverage in multiple bands by the Hubble Space Telescope
(HST) Multi-cycle Treasury Program CANDELS, S-CANDELS was carried out
within five widely separated extragalactic fields: the UKIDSS Ultra-deep
Survey, the Extended Chandra Deep Field South, COSMOS, the HST Deep
Field North, and the Extended Groth Strip. S-CANDELS builds upon the
existing coverage of these fields from the Spitzer Extended Deep Survey
(SEDS), a Cycle 6 Exploration Program, by increasing the integration
time from SEDS’ 12 hr to a total of 50 hr but within a smaller
area, 0.16 deg2. The additional depth significantly increases
the survey completeness at faint magnitudes. This paper describes the
S-CANDELS survey design, processing, and publicly available data
products. We present Infrared Array Camera (IRAC) dual-band 3.6+4.5 μ
\{\{m\}\} catalogs reaching to a depth of 26.5 AB mag. Deep IRAC counts for
the roughly 135,000 galaxies detected by S-CANDELS are consistent with
models based on known galaxy populations. The increase in depth beyond
earlier Spitzer/IRAC surveys does not reveal a significant additional
contribution from discrete sources to the diffuse Cosmic Infrared
Background (CIB). Thus it remains true that only roughly half of the
estimated CIB flux from COBE/DIRBE is resolved.},
	urldate = {2020-06-29},
	journal = {The Astrophysical Journal Supplement Series},
	author = {Ashby, M. L. N. and Willner, S. P. and Fazio, G. G. and Dunlop, J. S. and Egami, E. and Faber, S. M. and Ferguson, H. C. and Grogin, N. A. and Hora, J. L. and Huang, J.-S. and Koekemoer, A. M. and Labbé, I. and Wang, Z.},
	month = jun,
	year = {2015},
	keywords = {galaxies: high-redshift, infrared: galaxies, surveys},
	pages = {33}
}

@article{polletta_spectral_2007,
	title = {Spectral {Energy} {Distributions} of {Hard} {X}-{Ray} {Selected} {Active} {Galactic} {Nuclei} in the {XMM}-{Newton} {Medium} {Deep} {Survey}},
	volume = {663},
	issn = {0004-637X},
	url = {http://adsabs.harvard.edu/abs/2007ApJ...663...81P},
	doi = {10.1086/518113},
	abstract = {We present the SEDs of a hard X-ray selected sample containing 136 
sources with F2-10keV{\textgreater}10-14 erg cm-2
s-1 132 are AGNs. The sources are detected in a 1
deg2 area of the XMM-Newton Medium Deep Survey where optical
data from the VVDS and CFHTLS and infrared data from the SWIRE survey
are available. Based on a SED fitting technique we derive photometric
redshifts with σ(1+z)=0.11 and 6\% of outliers and identify AGN
signatures in 83\% of the objects. This fraction is higher than derived
when a spectroscopic classification is available. The remaining
17+9-6\% of AGNs show star-forming galaxy SEDs (SF
class). The sources with AGN signatures are divided in two classes, AGN1
(33+6-1\%) and AGN2
(50+6-11\%). The AGN1 and AGN2 classes include
sources whose SEDs are fitted by type 1 and type 2 AGN templates,
respectively. On average, AGN1s show soft X-ray spectra, consistent with
being unabsorbed, while AGN2s and SFs show hard X-ray spectra,
consistent with being absorbed. The analysis of the average SEDs as a
function of X-ray luminosity shows a reddening of the infrared SEDs,
consistent with a decreasing contribution from the host galaxy at higher
luminosities. The AGNs in the SF classes are likely obscured in the
mid-infrared, as suggested by their low
L3-20μm/Lcorr0.5-10keV ratios. We
confirm the previously found correlation for AGNs between the radio
luminosity and the X-ray and the mid-infrared luminosities. The
X-ray-radio correlation can be used to identify heavily absorbed AGNs.
However, the estimated radio fluxes for the missing AGN population
responsible for the bulk of the background at E{\textgreater}10 keV are too faint
to be detected even in the deepest current radio surveys.},
	urldate = {2020-06-29},
	journal = {The Astrophysical Journal},
	author = {Polletta, M. and Tajer, M. and Maraschi, L. and Trinchieri, G. and Lonsdale, C. J. and Chiappetti, L. and Andreon, S. and Pierre, M. and Le Fèvre, O. and Zamorani, G. and Maccagni, D. and Garcet, O. and Surdej, J. and Franceschini, A. and Alloin, D. and Shupe, D. L. and Surace, J. A. and Fang, F. and Rowan-Robinson, M. and Smith, H. E. and Tresse, L.},
	month = jul,
	year = {2007},
	keywords = {Galaxies: Active, Galaxies: Quasars: General, Infrared: Galaxies, X-Rays: Galaxies},
	pages = {81--102}
}

@article{bruzual_stellar_2003,
	title = {Stellar population synthesis at the resolution of 2003},
	volume = {344},
	issn = {0035-8711},
	url = {http://adsabs.harvard.edu/abs/2003MNRAS.344.1000B},
	doi = {10.1046/j.1365-8711.2003.06897.x},
	abstract = {We present a new model for computing the spectral evolution of stellar populations at ages between 1 × 105 and 2 ×
1010 yr at a resolution of 3 Å across the whole
wavelength range from 3200 to 9500 Å for a wide range of
metallicities. These predictions are based on a newly available library of observed stellar spectra. We also compute the spectral evolution across a larger wavelength range, from 91 Å to 160 μm, at lower
resolution. The model incorporates recent progress in stellar evolution theory and an observationally motivated prescription for thermally pulsing stars on the asymptotic giant branch. The latter is supported by observations of surface brightness fluctuations in nearby stellar populations. We show that this model reproduces well the observed optical and near-infrared colour-magnitude diagrams of Galactic star clusters of various ages and metallicities. Stochastic fluctuations in the numbers of stars in different evolutionary phases can account for the full range of observed integrated colours of star clusters in the Magellanic Clouds. The model reproduces in detail typical galaxy spectra from the Early Data Release (EDR) of the Sloan Digital Sky Survey (SDSS). We exemplify how this type of spectral fit can constrain physical parameters such as the star formation history, metallicity and dust content of galaxies. Our model is the first to enable accurate studies of absorption-line strengths in galaxies containing stars over the full range of ages. Using the highest-quality spectra of the SDSS EDR, we show that this model can reproduce simultaneously the observed strengths of those Lick indices that do not depend strongly on element abundance ratios. The interpretation of such indices with our model should be particularly useful for constraining the star formation histories and metallicities of galaxies.},
	urldate = {2020-06-29},
	journal = {Monthly Notices of the Royal Astronomical Society},
	author = {Bruzual, G. and Charlot, S.},
	month = oct,
	year = {2003},
	keywords = {galaxies: evolution, galaxies: formation, galaxies: stellar content, stars: evolution},
	pages = {1000--1028}
}

@article{calzetti_dust_2000,
	title = {The {Dust} {Content} and {Opacity} of {Actively} {Star}-forming {Galaxies}},
	volume = {533},
	issn = {0004-637X},
	url = {http://adsabs.harvard.edu/abs/2000ApJ...533..682C},
	doi = {10.1086/308692},
	abstract = {We present far-infrared (FIR) photometry at 150 and 205 μm of eight low-redshift starburst galaxies obtained with the Infrared Space Observatory (ISO) ISOPHOT. Five of the eight galaxies are detected in both wave bands, and these data are used, in conjunction with IRAS archival photometry, to model the dust emission at λ{\textgreater}{\textasciitilde}40
μm. The FIR spectral energy distributions (SEDs) are best fitted by a combination of two modified Planck functions, with T{\textasciitilde}40-55 K (warm dust) and T{\textasciitilde}20-23 K (cool dust) and with a dust emissivity index ɛ=2.
The cool dust can be a major contributor to the FIR emission of
starburst galaxies, representing up to 60\% of the total flux. This component is heated not only by the general interstellar radiation field, but also by the starburst itself. The cool dust mass is up to {\textasciitilde}150 times larger than the warm dust mass, bringing the gas-to-dust ratios of the starbursts in our sample close to Milky Way values, once rescaled for the appropriate metallicity. The ratio between the total dust FIR emission in the range 1-1000 μm and the IRAS FIR emission in the range 40-120 μm is {\textasciitilde}1.75, with small variations from galaxy to galaxy. This ratio is about 40\% larger than previously inferred from data at millimeter wavelengths. Although the galaxies in our sample are generally classified as ``UV bright,'' for four of them the UV energy emerging shortward of 0.2 μm is less than 15\% of the FIR energy. On average, about 30\% of the bolometric flux is coming out in the
UV-to-near-IR wavelength range; the rest is emitted in the FIR. Energy balance calculations show that the FIR emission predicted by the dust reddening of the UV-to-near-IR stellar emission is within a factor of {\textasciitilde}2 of the observed value in individual galaxies and within 20\% when averaged over a large sample. If our sample of local starbursts is representative of high-redshift (z{\textgreater}{\textasciitilde}1), UV-bright, star-forming
galaxies, these galaxies' FIR emission will be generally undetected in submillimeter surveys, unless (1) their bolometric luminosity is comparable to or larger than that of ultraluminous FIR galaxies and (2) their FIR SED contains a cool dust component. Based on observations with ISO, an ESA project with instruments funded by ESA member states (especially the PI countries: France, Germany, the Netherlands, and the United Kingdom) with the participation of ISAS and NASA.},
	urldate = {2020-06-29},
	journal = {The Astrophysical Journal},
	author = {Calzetti, Daniela and Armus, Lee and Bohlin, Ralph C. and Kinney, Anne L. and Koornneef, Jan and Storchi-Bergmann, Thaisa},
	month = apr,
	year = {2000},
	keywords = {EXTINCTION, GALAXIES: STARBURST, INFRARED: GALAXIES, INFRARED: ISM: CONTINUUM, ISM: DUST},
	pages = {682--695}
}

@article{prevot_typical_1984,
	title = {The typical interstellar extinction in the {Small} {Magellanic} {Cloud}},
	volume = {132},
	issn = {0004-6361},
	url = {http://adsabs.harvard.edu/abs/1984A%26A...132..389P},
	abstract = {The authors give a mean UV extinction curve for the Small Magellanic Cloud which corresponds to the most common case and consequently to the most probable typical extinction law. The curve is almost linear in λ-1 without any evidence of the 2200 Å galactic
feature. This is consistent with almost pure silicate interstellar grains and little graphite grains, as expected from the large
underabundance of carbon in the SMC with respect to other heavy
elements.},
	urldate = {2020-06-29},
	journal = {Astronomy and Astrophysics},
	author = {Prevot, M. L. and Lequeux, J. and Maurice, E. and Prevot, L. and Rocca-Volmerange, B.},
	month = mar,
	year = {1984},
	keywords = {Interstellar Extinction, Interstellar Matter, Iue, Magellanic Clouds, Ultraviolet Spectra},
	pages = {389--392}
}

@article{fitzpatrick_analysis_1986,
	title = {An analysis on the shapes of ultraviolet extinction curves. {I} - {The} 2175 {A} bump},
	volume = {307},
	issn = {0004-637X},
	url = {http://adsabs.harvard.edu/abs/1986ApJ...307..286F},
	doi = {10.1086/164415},
	abstract = {IUE data are used to investigate the properties of the 2175 A interstellar extinction bump toward 45 reddened Milky Way stars. Using analytic fitting functions, parameters are derived which describe the central position, FWHM, and strength of the bump. The bump position is very stable, with an extreme deviation which is still significantly larger than the measurement uncertainty, indicating true variability. The bump FWHM has a large range of intrinsic values, 0.77/micron to 1.25/micron. The normalized bump strength varies by more than a factor of three. There are no convincing correlations among the three bump parameters, but the width of the bump is strongly correlated with the dust grain environments. Dense quiescent regions yield broad bumps, while diffuse interstellar medium and regions of recent star formation yield narrower bumps. The absence of any correlation between bump width and central position argues strongly against graphite grains in the size range prescribed by the Mathis, Rumpl, and Nordsieck (1977) model as carriers of the bump.},
	urldate = {2020-06-29},
	journal = {The Astrophysical Journal},
	author = {Fitzpatrick, E. L. and Massa, D.},
	month = aug,
	year = {1986},
	keywords = {Interstellar Extinction, Interstellar Matter, Iue, Line Spectra, Milky Way Galaxy, Random Errors, Ultraviolet Spectra},
	pages = {286--294}
}

@ARTICLE{williams_hdf_96,
       author = {{Williams}, Robert E. and {Blacker}, Brett and {Dickinson}, Mark and
         {Dixon}, W. Van Dyke and {Ferguson}, Henry C. and
         {Fruchter}, Andrew S. and {Giavalisco}, Mauro and {Gilliland
        }, Ronald L. and {Heyer}, Inge and {Katsanis}, Rocio and {Levay}, Zolt and
         {Lucas}, Ray A. and {McElroy}, Douglas B. and {Petro}, Larry and
         {Postman}, Marc and {Adorf}, Hans-Martin and {Hook}, Richard},
        title = "{The Hubble Deep Field: Observations, Data Reduction, and Galaxy Photometry}",
      journal = {\aj},
     keywords = {GALAXIES: PHOTOMETRY, GALAXIES: EVOLUTION, Astrophysics},
         year = 1996,
        month = oct,
       volume = {112},
        pages = {1335},
          doi = {10.1086/118105},
archivePrefix = {arXiv},
       eprint = {astro-ph/9607174},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1996AJ....112.1335W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{whitaker20_goods_catalog,
       author = {{Whitaker}, Katherine E. and {Ashas}, Mohammad and {Illingworth}, Garth and
         {Magee}, Daniel and {Leja}, Joel and {Oesch}, Pascal and
         {van Dokkum}, Pieter and {Mowla}, Lamiya and {Bouwens}, Rychard and
         {Franx}, Marijn and {Holden}, Bradford and {Labb{\'e}}, Ivo and
         {Rafelski}, Marc and {Teplitz}, Harry and {Gonzalez}, Valentino},
        title = "{The Hubble Legacy Field GOODS-S Photometric Catalog}",
      journal = {\apjs},
     keywords = {catalogs, galaxies: evolution, galaxies: general, methods: data analysis, techniques: photometric, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = sep,
       volume = {244},
       number = {1},
          eid = {16},
        pages = {16},
          doi = {10.3847/1538-4365/ab3853},
archivePrefix = {arXiv},
       eprint = {1908.05682},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJS..244...16W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Illingworth13_hudf,
       author = {{Illingworth}, G.~D. and {Magee}, D. and {Oesch}, P.~A. and
         {Bouwens}, R.~J. and {Labb{\'e}}, I. and {Stiavelli}, M. and
         {van Dokkum}, P.~G. and {Franx}, M. and {Trenti}, M. and
         {Carollo}, C.~M. and {Gonzalez}, V.},
        title = "{The HST eXtreme Deep Field (XDF): Combining All ACS and WFC3/IR Data on the HUDF Region into the Deepest Field Ever}",
      journal = {\apjs},
     keywords = {cosmology: observations, galaxies: abundances, galaxies: high-redshift, techniques: image processing, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = nov,
       volume = {209},
       number = {1},
          eid = {6},
        pages = {6},
          doi = {10.1088/0067-0049/209/1/6},
archivePrefix = {arXiv},
       eprint = {1305.1931},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJS..209....6I},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{ishigaki18_UV_LF,
       author = {{Ishigaki}, Masafumi and {Kawamata}, Ryota and {Ouchi}, Masami and
         {Oguri}, Masamune and {Shimasaku}, Kazuhiro and {Ono}, Yoshiaki},
        title = "{Full-data Results of Hubble Frontier Fields: UV Luminosity Functions at z ̃ 6-10 and a Consistent Picture of Cosmic Reionization}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = feb,
       volume = {854},
       number = {1},
          eid = {73},
        pages = {73},
          doi = {10.3847/1538-4357/aaa544},
archivePrefix = {arXiv},
       eprint = {1702.04867},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ApJ...854...73I},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Robertson13_reionzation,
       author = {{Robertson}, Brant E. and {Furlanetto}, Steven R. and {Schneider}, Evan and
         {Charlot}, Stephane and {Ellis}, Richard S. and {Stark}, Daniel P. and
         {McLure}, Ross J. and {Dunlop}, James S. and {Koekemoer}, Anton and
         {Schenker}, Matthew A. and {Ouchi}, Masami and {Ono}, Yoshiaki and
         {Curtis-Lake}, Emma and {Rogers}, Alexander B. and
         {Bowler}, Rebecca A.~A. and {Cirasuolo}, Michele},
        title = "{New Constraints on Cosmic Reionization from the 2012 Hubble Ultra Deep Field Campaign}",
      journal = {\apj},
     keywords = {dark ages, reionization, first stars, galaxies: evolution, galaxies: formation, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = may,
       volume = {768},
       number = {1},
          eid = {71},
        pages = {71},
          doi = {10.1088/0004-637X/768/1/71},
archivePrefix = {arXiv},
       eprint = {1301.1228},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJ...768...71R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{salvato19_photoz_review,
        author = {{Salvato}, Mara and {Ilbert}, Olivier and {Hoyle}, Ben},
        title = "{The many flavours of photometric redshifts}",
      journal = {Nature Astronomy},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = jun,
       volume = {3},
        pages = {212-222},
          doi = {10.1038/s41550-018-0478-0},
archivePrefix = {arXiv},
       eprint = {1805.12574},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019NatAs...3..212S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{LSSTsciencebook,
       author = {{LSST Science Collaboration} and {Abell}, Paul A. and {Allison}, Julius and
         {Anderson}, Scott F. and {Andrew}, John R. and {Angel}, J. Roger P. and
         {Armus}, Lee and {Arnett}, David and {Asztalos}, S.~J. and
         {Axelrod}, Tim S. and {Bailey}, Stephen and {Ballantyne}, D.~R. and
         {Bankert}, Justin R. and {Barkhouse}, Wayne A. and {Barr}, Jeffrey D. and
         {Barrientos}, L. Felipe and {Barth}, Aaron J. and {Bartlett}, James G. and
         {Becker}, Andrew C. and {Becla}, Jacek and {Beers}, Timothy C. and
         {Bernstein}, Joseph P. and {Biswas}, Rahul and {Blanton}, Michael R. and
         {Bloom}, Joshua S. and {Bochanski}, John J. and {Boeshaar}, Pat and
         {Borne}, Kirk D. and {Bradac}, Marusa and {Brandt}, W.~N. and
         {Bridge}, Carrie R. and {Brown}, Michael E. and {Brunner}, Robert J. and
         {Bullock}, James S. and {Burgasser}, Adam J. and {Burge}, James H. and
         {Burke}, David L. and {Cargile}, Phillip A. and {Chand
        rasekharan}, Srinivasan and {Chartas}, George and {Chesley}, Steven R. and
         {Chu}, You-Hua and {Cinabro}, David and {Claire}, Mark W. and
         {Claver}, Charles F. and {Clowe}, Douglas and {Connolly}, A.~J. and
         {Cook}, Kem H. and {Cooke}, Jeff and {Cooray}, Asantha and
         {Covey}, Kevin R. and {Culliton}, Christopher S. and {de Jong}, Roelof and
         {de Vries}, Willem H. and {Debattista}, Victor P. and
         {Delgado}, Francisco and {Dell'Antonio}, Ian P. and {Dhital}, Saurav and
         {Di Stefano}, Rosanne and {Dickinson}, Mark and {Dilday}, Benjamin and
         {Djorgovski}, S.~G. and {Dobler}, Gregory and {Donalek}, Ciro and
         {Dubois-Felsmann}, Gregory and {Durech}, Josef and
         {Eliasdottir}, Ardis and {Eracleous}, Michael and {Eyer}, Laurent and
         {Falco}, Emilio E. and {Fan}, Xiaohui and {Fassnacht}, Christopher D. and
         {Ferguson}, Harry C. and {Fernandez}, Yanga R. and {Fields}, Brian D. and
         {Finkbeiner}, Douglas and {Figueroa}, Eduardo E. and {Fox}, Derek B. and
         {Francke}, Harold and {Frank}, James S. and {Frieman}, Josh and
         {Fromenteau}, Sebastien and {Furqan}, Muhammad and {Galaz}, Gaspar and
         {Gal-Yam}, A. and {Garnavich}, Peter and {Gawiser}, Eric and
         {Geary}, John and {Gee}, Perry and {Gibson}, Robert R. and
         {Gilmore}, Kirk and {Grace}, Emily A. and {Green}, Richard F. and
         {Gressler}, William J. and {Grillmair}, Carl J. and {Habib}, Salman and
         {Haggerty}, J.~S. and {Hamuy}, Mario and {Harris}, Alan W. and
         {Hawley}, Suzanne L. and {Heavens}, Alan F. and {Hebb}, Leslie and
         {Henry}, Todd J. and {Hileman}, Edward and {Hilton}, Eric J. and
         {Hoadley}, Keri and {Holberg}, J.~B. and {Holman}, Matt J. and
         {Howell}, Steve B. and {Infante}, Leopoldo and {Ivezic}, Zeljko and
         {Jacoby}, Suzanne H. and {Jain}, Bhuvnesh and {R} and {Jedicke} and
         {Jee}, M. James and {Garrett Jernigan}, J. and {Jha}, Saurabh W. and
         {Johnston}, Kathryn V. and {Jones}, R. Lynne and {Juric}, Mario and
         {Kaasalainen}, Mikko and {Styliani} and {Kafka} and {Kahn}, Steven M. and
         {Kaib}, Nathan A. and {Kalirai}, Jason and {Kantor}, Jeff and
         {Kasliwal}, Mansi M. and {Keeton}, Charles R. and {Kessler}, Richard and
         {Knezevic}, Zoran and {Kowalski}, Adam and {Krabbendam}, Victor L. and
         {Krughoff}, K. Simon and {Kulkarni}, Shrinivas and {Kuhlman}, Stephen and
         {Lacy}, Mark and {Lepine}, Sebastien and {Liang}, Ming and {Lien}, Amy and
         {Lira}, Paulina and {Long}, Knox S. and {Lorenz}, Suzanne and
         {Lotz}, Jennifer M. and {Lupton}, R.~H. and {Lutz}, Julie and
         {Macri}, Lucas M. and {Mahabal}, Ashish A. and {Mandelbaum}, Rachel and
         {Marshall}, Phil and {May}, Morgan and {McGehee}, Peregrine M. and
         {Meadows}, Brian T. and {Meert}, Alan and {Milani}, Andrea and
         {Miller}, Christopher J. and {Miller}, Michelle and {Mills}, David and
         {Minniti}, Dante and {Monet}, David and {Mukadam}, Anjum S. and
         {Nakar}, Ehud and {Neill}, Douglas R. and {Newman}, Jeffrey A. and
         {Nikolaev}, Sergei and {Nordby}, Martin and {O'Connor}, Paul and
         {Oguri}, Masamune and {Oliver}, John and {Olivier}, Scot S. and
         {Olsen}, Julia K. and {Olsen}, Knut and {Olszewski}, Edward W. and
         {Oluseyi}, Hakeem and {Padilla}, Nelson D. and {Parker}, Alex and
         {Pepper}, Joshua and {Peterson}, John R. and {Petry}, Catherine and
         {Pinto}, Philip A. and {Pizagno}, James L. and {Popescu}, Bogdan and
         {Prsa}, Andrej and {Radcka}, Veljko and {Raddick}, M. Jordan and
         {Rasmussen}, Andrew and {Rau}, Arne and {Rho}, Jeonghee and
         {Rhoads}, James E. and {Richards}, Gordon T. and {Ridgway}, Stephen T. and
         {Robertson}, Brant E. and {Roskar}, Rok and {Saha}, Abhijit and
         {Sarajedini}, Ata and {Scannapieco}, Evan and {Schalk}, Terry and
         {Schindler}, Rafe and {Schmidt}, Samuel and {Schmidt}, Sarah and
         {Schneider}, Donald P. and {Schumacher}, German and {Scranton}, Ryan and
         {Sebag}, Jacques and {Seppala}, Lynn G. and {Shemmer}, Ohad and
         {Simon}, Joshua D. and {Sivertz}, M. and {Smith}, Howard A. and
         {Allyn Smith}, J. and {Smith}, Nathan and {Spitz}, Anna H. and
         {Stanford}, Adam and {Stassun}, Keivan G. and {Strader}, Jay and
         {Strauss}, Michael A. and {Stubbs}, Christopher W. and
         {Sweeney}, Donald W. and {Szalay}, Alex and {Szkody}, Paula and
         {Takada}, Masahiro and {Thorman}, Paul and {Trilling}, David E. and
         {Trimble}, Virginia and {Tyson}, Anthony and {Van Berg}, Richard and {Vand
        en Berk}, Daniel and {VanderPlas}, Jake and {Verde}, Licia and
         {Vrsnak}, Bojan and {Walkowicz}, Lucianne M. and {Wand
        elt}, Benjamin D. and {Wang}, Sheng and {Wang}, Yun and
         {Warner}, Michael and {Wechsler}, Risa H. and {West}, Andrew A. and
         {Wiecha}, Oliver and {Williams}, Benjamin F. and {Willman}, Beth and
         {Wittman}, David and {Wolff}, Sidney C. and {Wood-Vasey}, W. Michael and
         {Wozniak}, Przemek and {Young}, Patrick and {Zentner}, Andrew and
         {Zhan}, Hu},
        title = "{LSST Science Book, Version 2.0}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Galaxy Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
         year = 2009,
        month = dec,
          eid = {arXiv:0912.0201},
        pages = {arXiv:0912.0201},
archivePrefix = {arXiv},
       eprint = {0912.0201},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009arXiv0912.0201L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}





@ARTICLE{laureijs11,
       author = {{Laureijs}, R. and {Amiaux}, J. and {Arduini}, S. and
         {Augu{\`e}res}, J. -L. and {Brinchmann}, J. and {Cole}, R. and
         {Cropper}, M. and {Dabin}, C. and {Duvet}, L. and {Ealet}, A. and
         {Garilli}, B. and {Gondoin}, P. and {Guzzo}, L. and {Hoar}, J. and
         {Hoekstra}, H. and {Holmes}, R. and {Kitching}, T. and {Maciaszek}, T. and
         {Mellier}, Y. and {Pasian}, F. and {Percival}, W. and {Rhodes}, J. and
         {Saavedra Criado}, G. and {Sauvage}, M. and {Scaramella}, R. and
         {Valenziano}, L. and {Warren}, S. and {Bender}, R. and {Castander}, F. and
         {Cimatti}, A. and {Le F{\`e}vre}, O. and {Kurki-Suonio}, H. and
         {Levi}, M. and {Lilje}, P. and {Meylan}, G. and {Nichol}, R. and
         {Pedersen}, K. and {Popa}, V. and {Rebolo Lopez}, R. and {Rix}, H. -W. and
         {Rottgering}, H. and {Zeilinger}, W. and {Grupp}, F. and {Hudelot}, P. and
         {Massey}, R. and {Meneghetti}, M. and {Miller}, L. and {Paltani}, S. and
         {Paulin-Henriksson}, S. and {Pires}, S. and {Saxton}, C. and
         {Schrabback}, T. and {Seidel}, G. and {Walsh}, J. and {Aghanim}, N. and
         {Amendola}, L. and {Bartlett}, J. and {Baccigalupi}, C. and
         {Beaulieu}, J. -P. and {Benabed}, K. and {Cuby}, J. -G. and
         {Elbaz}, D. and {Fosalba}, P. and {Gavazzi}, G. and {Helmi}, A. and
         {Hook}, I. and {Irwin}, M. and {Kneib}, J. -P. and {Kunz}, M. and
         {Mannucci}, F. and {Moscardini}, L. and {Tao}, C. and {Teyssier}, R. and
         {Weller}, J. and {Zamorani}, G. and {Zapatero Osorio}, M.~R. and
         {Boulade}, O. and {Foumond}, J.~J. and {Di Giorgio}, A. and
         {Guttridge}, P. and {James}, A. and {Kemp}, M. and {Martignac}, J. and
         {Spencer}, A. and {Walton}, D. and {Bl{\"u}mchen}, T. and {Bonoli}, C. and
         {Bortoletto}, F. and {Cerna}, C. and {Corcione}, L. and {Fabron}, C. and
         {Jahnke}, K. and {Ligori}, S. and {Madrid}, F. and {Martin}, L. and
         {Morgante}, G. and {Pamplona}, T. and {Prieto}, E. and {Riva}, M. and
         {Toledo}, R. and {Trifoglio}, M. and {Zerbi}, F. and {Abdalla}, F. and
         {Douspis}, M. and {Grenet}, C. and {Borgani}, S. and {Bouwens}, R. and
         {Courbin}, F. and {Delouis}, J. -M. and {Dubath}, P. and {Fontana}, A. and
         {Frailis}, M. and {Grazian}, A. and {Koppenh{\"o}fer}, J. and
         {Mansutti}, O. and {Melchior}, M. and {Mignoli}, M. and {Mohr}, J. and
         {Neissner}, C. and {Noddle}, K. and {Poncet}, M. and {Scodeggio}, M. and
         {Serrano}, S. and {Shane}, N. and {Starck}, J. -L. and {Surace}, C. and
         {Taylor}, A. and {Verdoes-Kleijn}, G. and {Vuerli}, C. and
         {Williams}, O.~R. and {Zacchei}, A. and {Altieri}, B. and
         {Escudero Sanz}, I. and {Kohley}, R. and {Oosterbroek}, T. and
         {Astier}, P. and {Bacon}, D. and {Bardelli}, S. and {Baugh}, C. and
         {Bellagamba}, F. and {Benoist}, C. and {Bianchi}, D. and {Biviano}, A. and
         {Branchini}, E. and {Carbone}, C. and {Cardone}, V. and {Clements}, D. and
         {Colombi}, S. and {Conselice}, C. and {Cresci}, G. and {Deacon}, N. and
         {Dunlop}, J. and {Fedeli}, C. and {Fontanot}, F. and {Franzetti}, P. and
         {Giocoli}, C. and {Garcia-Bellido}, J. and {Gow}, J. and {Heavens}, A. and
         {Hewett}, P. and {Heymans}, C. and {Holland}, A. and {Huang}, Z. and
         {Ilbert}, O. and {Joachimi}, B. and {Jennins}, E. and {Kerins}, E. and
         {Kiessling}, A. and {Kirk}, D. and {Kotak}, R. and {Krause}, O. and
         {Lahav}, O. and {van Leeuwen}, F. and {Lesgourgues}, J. and
         {Lombardi}, M. and {Magliocchetti}, M. and {Maguire}, K. and
         {Majerotto}, E. and {Maoli}, R. and {Marulli}, F. and
         {Maurogordato}, S. and {McCracken}, H. and {McLure}, R. and
         {Melchiorri}, A. and {Merson}, A. and {Moresco}, M. and {Nonino}, M. and
         {Norberg}, P. and {Peacock}, J. and {Pello}, R. and {Penny}, M. and
         {Pettorino}, V. and {Di Porto}, C. and {Pozzetti}, L. and
         {Quercellini}, C. and {Radovich}, M. and {Rassat}, A. and {Roche}, N. and
         {Ronayette}, S. and {Rossetti}, E. and {Sartoris}, B. and
         {Schneider}, P. and {Semboloni}, E. and {Serjeant}, S. and
         {Simpson}, F. and {Skordis}, C. and {Smadja}, G. and {Smartt}, S. and
         {Spano}, P. and {Spiro}, S. and {Sullivan}, M. and {Tilquin}, A. and
         {Trotta}, R. and {Verde}, L. and {Wang}, Y. and {Williger}, G. and
         {Zhao}, G. and {Zoubian}, J. and {Zucca}, E.},
        title = "{Euclid Definition Study Report}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - Galaxy Astrophysics},
         year = 2011,
        month = oct,
          eid = {arXiv:1110.3193},
        pages = {arXiv:1110.3193},
archivePrefix = {arXiv},
       eprint = {1110.3193},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011arXiv1110.3193L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{hildebrandt17_kids,
   author = {{Hildebrandt}, H. and {Viola}, M. and {Heymans}, C. and {Joudaki}, S. and 
	{Kuijken}, K. and {Blake}, C. and {Erben}, T. and {Joachimi}, B. and 
	{Klaes}, D. and {Miller}, L. and {Morrison}, C.~B. and {Nakajima}, R. and 
	{Verdoes Kleijn}, G. and {Amon}, A. and {Choi}, A. and {Covone}, G. and 
	{de Jong}, J.~T.~A. and {Dvornik}, A. and {Fenech Conti}, I. and 
	{Grado}, A. and {Harnois-D{\'e}raps}, J. and {Herbonnet}, R. and 
	{Hoekstra}, H. and {K{\"o}hlinger}, F. and {McFarland}, J. and 
	{Mead}, A. and {Merten}, J. and {Napolitano}, N. and {Peacock}, J.~A. and 
	{Radovich}, M. and {Schneider}, P. and {Simon}, P. and {Valentijn}, E.~A. and 
	{van den Busch}, J.~L. and {van Uitert}, E. and {Van Waerbeke}, L.
	},
    title = "{KiDS-450: cosmological parameter constraints from tomographic weak gravitational lensing}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1606.05338},
 keywords = {gravitational lensing: weak, surveys, galaxies: photometry, cosmology: observations},
     year = 2017,
    month = feb,
   volume = 465,
    pages = {1454-1498},
      doi = {10.1093/mnras/stw2805},
   adsurl = {http://cdsads.u-strasbg.fr/abs/2017MNRAS.465.1454H},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{troxel18_DES,
       author = {{Troxel}, M.~A. and {MacCrann}, N. and {Zuntz}, J. and {Eifler}, T.~F. and
         {Krause}, E. and {Dodelson}, S. and {Gruen}, D. and {Blazek}, J. and
         {Friedrich}, O. and {Samuroff}, S. and {Prat}, J. and {Secco}, L.~F. and
         {Davis}, C. and {Fert{\'e}}, A. and {DeRose}, J. and {Alarcon}, A. and
         {Amara}, A. and {Baxter}, E. and {Becker}, M.~R. and
         {Bernstein}, G.~M. and {Bridle}, S.~L. and {Cawthon}, R. and
         {Chang}, C. and {Choi}, A. and {De Vicente}, J. and
         {Drlica-Wagner}, A. and {Elvin-Poole}, J. and {Frieman}, J. and
         {Gatti}, M. and {Hartley}, W.~G. and {Honscheid}, K. and {Hoyle}, B. and
         {Huff}, E.~M. and {Huterer}, D. and {Jain}, B. and {Jarvis}, M. and
         {Kacprzak}, T. and {Kirk}, D. and {Kokron}, N. and {Krawiec}, C. and
         {Lahav}, O. and {Liddle}, A.~R. and {Peacock}, J. and {Rau}, M.~M. and
         {Refregier}, A. and {Rollins}, R.~P. and {Rozo}, E. and
         {Rykoff}, E.~S. and {S{\'a}nchez}, C. and {Sevilla-Noarbe}, I. and
         {Sheldon}, E. and {Stebbins}, A. and {Varga}, T.~N. and {Vielzeuf}, P. and
         {Wang}, M. and {Wechsler}, R.~H. and {Yanny}, B. and
         {Abbott}, T.~M.~C. and {Abdalla}, F.~B. and {Allam}, S. and
         {Annis}, J. and {Bechtol}, K. and {Benoit-L{\'e}vy}, A. and
         {Bertin}, E. and {Brooks}, D. and {Buckley-Geer}, E. and
         {Burke}, D.~L. and {Carnero Rosell}, A. and {Carrasco Kind}, M. and
         {Carretero}, J. and {Castander}, F.~J. and {Crocce}, M. and
         {Cunha}, C.~E. and {D'Andrea}, C.~B. and {da Costa}, L.~N. and
         {DePoy}, D.~L. and {Desai}, S. and {Diehl}, H.~T. and
         {Dietrich}, J.~P. and {Doel}, P. and {Fernandez}, E. and
         {Flaugher}, B. and {Fosalba}, P. and {Garc{\'\i}a-Bellido}, J. and
         {Gaztanaga}, E. and {Gerdes}, D.~W. and {Giannantonio}, T. and
         {Goldstein}, D.~A. and {Gruendl}, R.~A. and {Gschwend}, J. and
         {Gutierrez}, G. and {James}, D.~J. and {Jeltema}, T. and
         {Johnson}, M.~W.~G. and {Johnson}, M.~D. and {Kent}, S. and
         {Kuehn}, K. and {Kuhlmann}, S. and {Kuropatkin}, N. and {Li}, T.~S. and
         {Lima}, M. and {Lin}, H. and {Maia}, M.~A.~G. and {March}, M. and
         {Marshall}, J.~L. and {Martini}, P. and {Melchior}, P. and
         {Menanteau}, F. and {Miquel}, R. and {Mohr}, J.~J. and {Neilsen}, E. and
         {Nichol}, R.~C. and {Nord}, B. and {Petravick}, D. and {Plazas}, A.~A. and
         {Romer}, A.~K. and {Roodman}, A. and {Sako}, M. and {Sanchez}, E. and
         {Scarpine}, V. and {Schindler}, R. and {Schubnell}, M. and {Smith}, M. and
         {Smith}, R.~C. and {Soares-Santos}, M. and {Sobreira}, F. and
         {Suchyta}, E. and {Swanson}, M.~E.~C. and {Tarle}, G. and {Thomas}, D. and
         {Tucker}, D.~L. and {Vikram}, V. and {Walker}, A.~R. and {Weller}, J. and
         {Zhang}, Y. and {DES Collaboration}},
        title = "{Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear}",
      journal = {\prd},
     keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2018,
        month = aug,
       volume = {98},
       number = {4},
          eid = {043528},
        pages = {043528},
          doi = {10.1103/PhysRevD.98.043528},
archivePrefix = {arXiv},
       eprint = {1708.01538},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018PhRvD..98d3528T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{hikage19_hsc,
       author = {{Hikage}, Chiaki and {Oguri}, Masamune and {Hamana}, Takashi and
         {More}, Surhud and {Mandelbaum}, Rachel and {Takada}, Masahiro and
         {K{\"o}hlinger}, Fabian and {Miyatake}, Hironao and
         {Nishizawa}, Atsushi J. and {Aihara}, Hiroaki and {Armstrong}, Robert and
         {Bosch}, James and {Coupon}, Jean and {Ducout}, Anne and {Ho}, Paul and
         {Hsieh}, Bau-Ching and {Komiyama}, Yutaka and
         {Lanusse}, Fran{\c{c}}ois and {Leauthaud}, Alexie and
         {Lupton}, Robert H. and {Medezinski}, Elinor and {Mineo}, Sogo and
         {Miyama}, Shoken and {Miyazaki}, Satoshi and {Murata}, Ryoma and
         {Murayama}, Hitoshi and {Shirasaki}, Masato and
         {Sif{\'o}n}, Crist{\'o}bal and {Simet}, Melanie and {Speagle}, Joshua and
         {Spergel}, David N. and {Strauss}, Michael A. and {Sugiyama}, Naoshi and
         {Tanaka}, Masayuki and {Utsumi}, Yousuke and {Wang}, Shiang-Yu and
         {Yamada}, Yoshihiko},
        title = "{Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data}",
      journal = {\pasj},
     keywords = {dark matter, gravitational lensing: weak, large-scale structure of universe, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2019,
        month = apr,
       volume = {71},
       number = {2},
          eid = {43},
        pages = {43},
          doi = {10.1093/pasj/psz010},
archivePrefix = {arXiv},
       eprint = {1809.09148},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019PASJ...71...43H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{scoville07_hst,
       author = {{Scoville}, N. and {Abraham}, R.~G. and {Aussel}, H. and
         {Barnes}, J.~E. and {Benson}, A. and {Blain}, A.~W. and {Calzetti}, D. and
         {Comastri}, A. and {Capak}, P. and {Carilli}, C. and
         {Carlstrom}, J.~E. and {Carollo}, C.~M. and {Colbert}, J. and
         {Daddi}, E. and {Ellis}, R.~S. and {Elvis}, M. and {Ewald}, S.~P. and
         {Fall}, M. and {Franceschini}, A. and {Giavalisco}, M. and {Green}, W. and
         {Griffiths}, R.~E. and {Guzzo}, L. and {Hasinger}, G. and {Impey}, C. and
         {Kneib}, J. -P. and {Koda}, J. and {Koekemoer}, A. and {Lefevre}, O. and
         {Lilly}, S. and {Liu}, C.~T. and {McCracken}, H.~J. and {Massey}, R. and
         {Mellier}, Y. and {Miyazaki}, S. and {Mobasher}, B. and {Mould}, J. and
         {Norman}, C. and {Refregier}, A. and {Renzini}, A. and {Rhodes}, J. and
         {Rich}, M. and {Sanders}, D.~B. and {Schiminovich}, D. and
         {Schinnerer}, E. and {Scodeggio}, M. and {Sheth}, K. and
         {Shopbell}, P.~L. and {Taniguchi}, Y. and {Tyson}, N.~D. and
         {Urry}, C.~M. and {Van Waerbeke}, L. and {Vettolani}, P. and
         {White}, S.~D.~M. and {Yan}, L.},
        title = "{COSMOS: Hubble Space Telescope Observations}",
      journal = {\apjs},
     keywords = {Cosmology: Observations, Cosmology: Dark Matter, Galaxies: Evolution, Galaxies: Formation, Cosmology: Large-Scale Structure of Universe, Surveys, Astrophysics},
         year = 2007,
        month = sep,
       volume = {172},
       number = {1},
        pages = {38-45},
          doi = {10.1086/516580},
archivePrefix = {arXiv},
       eprint = {astro-ph/0612306},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007ApJS..172...38S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{civano16_chandra,
       author = {{Civano}, F. and {Marchesi}, S. and {Comastri}, A. and {Urry}, M.~C. and
         {Elvis}, M. and {Cappelluti}, N. and {Puccetti}, S. and {Brusa}, M. and
         {Zamorani}, G. and {Hasinger}, G. and {Aldcroft}, T. and {Alexand
        er}, D.~M. and {Allevato}, V. and {Brunner}, H. and {Capak}, P. and
         {Finoguenov}, A. and {Fiore}, F. and {Fruscione}, A. and {Gilli}, R. and
         {Glotfelty}, K. and {Griffiths}, R.~E. and {Hao}, H. and
         {Harrison}, F.~A. and {Jahnke}, K. and {Kartaltepe}, J. and
         {Karim}, A. and {LaMassa}, S.~M. and {Lanzuisi}, G. and {Miyaji}, T. and
         {Ranalli}, P. and {Salvato}, M. and {Sargent}, M. and
         {Scoville}, N.~J. and {Schawinski}, K. and {Schinnerer}, E. and
         {Silverman}, J. and {Smolcic}, V. and {Stern}, D. and {Toft}, S. and
         {Trakhtenbrot}, B. and {Treister}, E. and {Vignali}, C.},
        title = "{The Chandra Cosmos Legacy Survey: Overview and Point Source Catalog}",
      journal = {\apj},
     keywords = {catalogs, cosmology: observations, galaxies: evolution, quasars: general, surveys, X-rays: general, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = mar,
       volume = {819},
       number = {1},
          eid = {62},
        pages = {62},
          doi = {10.3847/0004-637X/819/1/62},
archivePrefix = {arXiv},
       eprint = {1601.00941},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016ApJ...819...62C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{smolcic17_radio,
       author = {{Smol{\v{c}}i{\'c}}, V. and {Novak}, M. and {Bondi}, M. and
         {Ciliegi}, P. and {Mooley}, K.~P. and {Schinnerer}, E. and
         {Zamorani}, G. and {Navarrete}, F. and {Bourke}, S. and {Karim}, A. and
         {Vardoulaki}, E. and {Leslie}, S. and {Delhaize}, J. and
         {Carilli}, C.~L. and {Myers}, S.~T. and {Baran}, N. and
         {Delvecchio}, I. and {Miettinen}, O. and {Banfield}, J. and
         {Balokovi{\'c}}, M. and {Bertoldi}, F. and {Capak}, P. and
         {Frail}, D.~A. and {Hallinan}, G. and {Hao}, H. and {Herrera Ruiz}, N. and
         {Horesh}, A. and {Ilbert}, O. and {Intema}, H. and {Jeli{\'c}}, V. and
         {Kl{\"o}ckner}, H. -R. and {Krpan}, J. and {Kulkarni}, S.~R. and
         {McCracken}, H. and {Laigle}, C. and {Middleberg}, E. and
         {Murphy}, E.~J. and {Sargent}, M. and {Scoville}, N.~Z. and {Sheth}, K.},
        title = "{The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release}",
      journal = {\aap},
     keywords = {catalogs, cosmology: observations, radio continuum: galaxies, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = jun,
       volume = {602},
          eid = {A1},
        pages = {A1},
          doi = {10.1051/0004-6361/201628704},
archivePrefix = {arXiv},
       eprint = {1703.09713},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017A&A...602A...1S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{bowler20_z8-10,
       author = {{Bowler}, R.~A.~A. and {Jarvis}, M.~J. and {Dunlop}, J.~S. and
         {McLure}, R.~J. and {McLeod}, D.~J. and {Adams}, N.~J. and
         {Milvang-Jensen}, B. and {McCracken}, H.~J.},
        title = "{A lack of evolution in the very bright end of the galaxy luminosity function from z ≃ 8 to 10}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2020,
        month = apr,
       volume = {493},
       number = {2},
        pages = {2059-2084},
          doi = {10.1093/mnras/staa313},
archivePrefix = {arXiv},
       eprint = {1911.12832},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.493.2059B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{laigle18_filaments,
       author = {{Laigle}, C. and {Pichon}, C. and {Arnouts}, S. and {McCracken}, H.~J. and
         {Dubois}, Y. and {Devriendt}, J. and {Slyz}, A. and {Le Borgne}, D. and
         {Benoit-L{\'e}vy}, A. and {Hwang}, Ho Seong and {Ilbert}, O. and
         {Kraljic}, K. and {Malavasi}, N. and {Park}, Changbom and {Vibert}, D.},
        title = "{COSMOS2015 photometric redshifts probe the impact of filaments on galaxy properties}",
      journal = {\mnras},
     keywords = {methods: numerical, methods: observational, techniques: photometric, galaxies: evolution, galaxies: formation, large-scale structure of Universe, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2018,
        month = mar,
       volume = {474},
       number = {4},
        pages = {5437-5458},
          doi = {10.1093/mnras/stx3055},
archivePrefix = {arXiv},
       eprint = {1702.08810},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.474.5437L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{scoville13_cosmicweb,
       author = {{Scoville}, N. and {Arnouts}, S. and {Aussel}, H. and {Benson}, A. and
         {Bongiorno}, A. and {Bundy}, K. and {Calvo}, M.~A.~A. and {Capak}, P. and
         {Carollo}, M. and {Civano}, F. and {Dunlop}, J. and {Elvis}, M. and
         {Faisst}, A. and {Finoguenov}, A. and {Fu}, Hai and {Giavalisco}, M. and
         {Guo}, Q. and {Ilbert}, O. and {Iovino}, A. and {Kajisawa}, M. and
         {Kartaltepe}, J. and {Leauthaud}, A. and {Le F{\`e}vre}, O. and
         {LeFloch}, E. and {Lilly}, S.~J. and {Liu}, C.~T. -C. and
         {Manohar}, S. and {Massey}, R. and {Masters}, D. and
         {McCracken}, H.~J. and {Mobasher}, B. and {Peng}, Y. -J. and
         {Renzini}, A. and {Rhodes}, J. and {Salvato}, M. and {Sanders}, D.~B. and
         {Sarvestani}, B.~D. and {Scarlata}, C. and {Schinnerer}, E. and
         {Sheth}, K. and {Shopbell}, P.~L. and {Smol{\v{c}}i{\'c}}, V. and
         {Taniguchi}, Y. and {Taylor}, J.~E. and {White}, S.~D.~M. and {Yan}, L.},
        title = "{Evolution of Galaxies and Their Environments at z = 0.1-3 in COSMOS}",
      journal = {\apjs},
     keywords = {galaxies: evolution, large-scale structure of universe, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = may,
       volume = {206},
       number = {1},
          eid = {3},
        pages = {3},
          doi = {10.1088/0067-0049/206/1/3},
archivePrefix = {arXiv},
       eprint = {1303.6689},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJS..206....3S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{muzzin13_mass,
       author = {{Muzzin}, Adam and {Marchesini}, Danilo and {Stefanon}, Mauro and
         {Franx}, Marijn and {McCracken}, Henry J. and {Milvang-Jensen}, Bo and
         {Dunlop}, James S. and {Fynbo}, J.~P.~U. and {Brammer}, Gabriel and
         {Labb{\'e}}, Ivo and {van Dokkum}, Pieter G.},
        title = "{The Evolution of the Stellar Mass Functions of Star-forming and Quiescent Galaxies to z = 4 from the COSMOS/UltraVISTA Survey}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: fundamental parameters, galaxies: high-redshift, galaxies: luminosity function, mass function, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = nov,
       volume = {777},
       number = {1},
          eid = {18},
        pages = {18},
          doi = {10.1088/0004-637X/777/1/18},
archivePrefix = {arXiv},
       eprint = {1303.4409},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJ...777...18M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Davidzon17_mass,
       author = {{Davidzon}, I. and {Ilbert}, O. and {Laigle}, C. and {Coupon}, J. and
         {McCracken}, H.~J. and {Delvecchio}, I. and {Masters}, D. and
         {Capak}, P. and {Hsieh}, B.~C. and {Le F{\`e}vre}, O. and {Tresse}, L. and
         {Bethermin}, M. and {Chang}, Y. -Y. and {Faisst}, A.~L. and
         {Le Floc'h}, E. and {Steinhardt}, C. and {Toft}, S. and {Aussel}, H. and
         {Dubois}, C. and {Hasinger}, G. and {Salvato}, M. and {Sanders}, D.~B. and
         {Scoville}, N. and {Silverman}, J.~D.},
        title = "{The COSMOS2015 galaxy stellar mass function . Thirteen billion years of stellar mass assembly in ten snapshots}",
      journal = {\aap},
     keywords = {galaxies: evolution, galaxies: luminosity function, mass function, galaxies: statistics, galaxies: high-redshift, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2017,
        month = sep,
       volume = {605},
          eid = {A70},
        pages = {A70},
          doi = {10.1051/0004-6361/201730419},
archivePrefix = {arXiv},
       eprint = {1701.02734},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017A&A...605A..70D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Ilbert15_ssfr,
       author = {{Ilbert}, O. and {Arnouts}, S. and {Le Floc'h}, E. and {Aussel}, H. and
         {Bethermin}, M. and {Capak}, P. and {Hsieh}, B. -C. and {Kajisawa}, M. and
         {Karim}, A. and {Le F{\`e}vre}, O. and {Lee}, N. and {Lilly}, S. and
         {McCracken}, H.~J. and {Michel-Dansac}, L. and {Moutard}, T. and
         {Renzini}, M.~A. and {Salvato}, M. and {Sanders}, D.~B. and
         {Scoville}, N. and {Sheth}, K. and {Silverman}, J.~D. and
         {Smol{\v{c}}i{\'c}}, V. and {Taniguchi}, Y. and {Tresse}, L.},
        title = "{Evolution of the specific star formation rate function at z\&lt; 1.4 Dissecting the mass-SFR plane in COSMOS and GOODS}",
      journal = {\aap},
     keywords = {galaxies: evolution, galaxies: luminosity function, mass function, galaxies: stellar content, galaxies: star formation, galaxies: statistics, galaxies: formation, Astrophysics - Astrophysics of Galaxies},
         year = 2015,
        month = jul,
       volume = {579},
          eid = {A2},
        pages = {A2},
          doi = {10.1051/0004-6361/201425176},
archivePrefix = {arXiv},
       eprint = {1410.4875},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015A&A...579A...2I},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{gruppioni13_LF_IR,
       author = {{Gruppioni}, C. and {Pozzi}, F. and {Rodighiero}, G. and
         {Delvecchio}, I. and {Berta}, S. and {Pozzetti}, L. and {Zamorani}, G. and
         {Andreani}, P. and {Cimatti}, A. and {Ilbert}, O. and {Le Floc'h}, E. and
         {Lutz}, D. and {Magnelli}, B. and {Marchetti}, L. and {Monaco}, P. and
         {Nordon}, R. and {Oliver}, S. and {Popesso}, P. and {Riguccini}, L. and
         {Roseboom}, I. and {Rosario}, D.~J. and {Sargent}, M. and
         {Vaccari}, M. and {Altieri}, B. and {Aussel}, H. and {Bongiovanni}, A. and
         {Cepa}, J. and {Daddi}, E. and {Dom{\'\i}nguez-S{\'a}nchez}, H. and
         {Elbaz}, D. and {F{\"o}rster Schreiber}, N. and {Genzel}, R. and
         {Iribarrem}, A. and {Magliocchetti}, M. and {Maiolino}, R. and
         {Poglitsch}, A. and {P{\'e}rez Garc{\'\i}a}, A. and
         {Sanchez-Portal}, M. and {Sturm}, E. and {Tacconi}, L. and
         {Valtchanov}, I. and {Amblard}, A. and {Arumugam}, V. and
         {Bethermin}, M. and {Bock}, J. and {Boselli}, A. and {Buat}, V. and
         {Burgarella}, D. and {Castro-Rodr{\'\i}guez}, N. and {Cava}, A. and
         {Chanial}, P. and {Clements}, D.~L. and {Conley}, A. and {Cooray}, A. and
         {Dowell}, C.~D. and {Dwek}, E. and {Eales}, S. and {Franceschini}, A. and
         {Glenn}, J. and {Griffin}, M. and {Hatziminaoglou}, E. and {Ibar}, E. and
         {Isaak}, K. and {Ivison}, R.~J. and {Lagache}, G. and {Levenson}, L. and
         {Lu}, N. and {Madden}, S. and {Maffei}, B. and {Mainetti}, G. and
         {Nguyen}, H.~T. and {O'Halloran}, B. and {Page}, M.~J. and
         {Panuzzo}, P. and {Papageorgiou}, A. and {Pearson}, C.~P. and
         {P{\'e}rez-Fournon}, I. and {Pohlen}, M. and {Rigopoulou}, D. and
         {Rowan-Robinson}, M. and {Schulz}, B. and {Scott}, D. and
         {Seymour}, N. and {Shupe}, D.~L. and {Smith}, A.~J. and
         {Stevens}, J.~A. and {Symeonidis}, M. and {Trichas}, M. and
         {Tugwell}, K.~E. and {Vigroux}, L. and {Wang}, L. and {Wright}, G. and
         {Xu}, C.~K. and {Zemcov}, M. and {Bardelli}, S. and {Carollo}, M. and
         {Contini}, T. and {Le F{\'e}vre}, O. and {Lilly}, S. and
         {Mainieri}, V. and {Renzini}, A. and {Scodeggio}, M. and {Zucca}, E.},
        title = "{The Herschel PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4}",
      journal = {\mnras},
     keywords = {galaxies: active, galaxies: evolution, galaxies: luminosity function, mass function, galaxies: starburst, cosmology: observations, infrared: galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = jun,
       volume = {432},
       number = {1},
        pages = {23-52},
          doi = {10.1093/mnras/stt308},
archivePrefix = {arXiv},
       eprint = {1302.5209},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013MNRAS.432...23G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{rodighiero11_massSFR,
       author = {{Rodighiero}, G. and {Daddi}, E. and {Baronchelli}, I. and
         {Cimatti}, A. and {Renzini}, A. and {Aussel}, H. and {Popesso}, P. and
         {Lutz}, D. and {Andreani}, P. and {Berta}, S. and {Cava}, A. and
         {Elbaz}, D. and {Feltre}, A. and {Fontana}, A. and
         {F{\"o}rster Schreiber}, N.~M. and {Franceschini}, A. and {Genzel}, R. and
         {Grazian}, A. and {Gruppioni}, C. and {Ilbert}, O. and {Le Floch}, E. and
         {Magdis}, G. and {Magliocchetti}, M. and {Magnelli}, B. and
         {Maiolino}, R. and {McCracken}, H. and {Nordon}, R. and
         {Poglitsch}, A. and {Santini}, P. and {Pozzi}, F. and {Riguccini}, L. and
         {Tacconi}, L.~J. and {Wuyts}, S. and {Zamorani}, G.},
        title = "{The Lesser Role of Starbursts in Star Formation at z = 2}",
      journal = {\apjl},
     keywords = {galaxies: evolution, galaxies: interactions, galaxies: nuclei, galaxies: starburst, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2011,
        month = oct,
       volume = {739},
       number = {2},
          eid = {L40},
        pages = {L40},
          doi = {10.1088/2041-8205/739/2/L40},
archivePrefix = {arXiv},
       eprint = {1108.0933},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJ...739L..40R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{peng10_quenching,
       author = {{Peng}, Ying-jie and {Lilly}, Simon J. and {Kova{\v{c}}}, Katarina and
         {Bolzonella}, Micol and {Pozzetti}, Lucia and {Renzini}, Alvio and
         {Zamorani}, Gianni and {Ilbert}, Olivier and {Knobel}, Christian and
         {Iovino}, Angela and {Maier}, Christian and {Cucciati}, Olga and
         {Tasca}, Lidia and {Carollo}, C. Marcella and {Silverman}, John and
         {Kampczyk}, Pawel and {de Ravel}, Loic and {Sanders}, David and
         {Scoville}, Nicholas and {Contini}, Thierry and {Mainieri}, Vincenzo and
         {Scodeggio}, Marco and {Kneib}, Jean-Paul and {Le F{\`e}vre}, Olivier and
         {Bardelli}, Sandro and {Bongiorno}, Angela and {Caputi}, Karina and
         {Coppa}, Graziano and {de la Torre}, Sylvain and {Franzetti}, Paolo and
         {Garilli}, Bianca and {Lamareille}, Fabrice and
         {Le Borgne}, Jean-Francois and {Le Brun}, Vincent and {Mignoli}, Marco and
         {Perez Montero}, Enrique and {Pello}, Roser and {Ricciardelli}, Elena and
         {Tanaka}, Masayuki and {Tresse}, Laurence and {Vergani}, Daniela and
         {Welikala}, Niraj and {Zucca}, Elena and {Oesch}, Pascal and
         {Abbas}, Ummi and {Barnes}, Luke and {Bordoloi}, Rongmon and
         {Bottini}, Dario and {Cappi}, Alberto and {Cassata}, Paolo and
         {Cimatti}, Andrea and {Fumana}, Marco and {Hasinger}, Gunther and
         {Koekemoer}, Anton and {Leauthaud}, Alexei and {Maccagni}, Dario and
         {Marinoni}, Christian and {McCracken}, Henry and {Memeo}, Pierdomenico and
         {Meneux}, Baptiste and {Nair}, Preethi and {Porciani}, Cristiano and
         {Presotto}, Valentina and {Scaramella}, Roberto},
        title = "{Mass and Environment as Drivers of Galaxy Evolution in SDSS and zCOSMOS and the Origin of the Schechter Function}",
      journal = {\apj},
     keywords = {cosmology: observations, galaxies: active, galaxies: distances and redshifts, galaxies: evolution, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2010,
        month = sep,
       volume = {721},
       number = {1},
        pages = {193-221},
          doi = {10.1088/0004-637X/721/1/193},
archivePrefix = {arXiv},
       eprint = {1003.4747},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010ApJ...721..193P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{daddi04,
       author = {{Daddi}, E. and {Cimatti}, A. and {Renzini}, A. and {Fontana}, A. and {Mignoli}, M. and {Pozzetti}, L. and {Tozzi}, P. and {Zamorani}, G.},
        title = "{A New Photometric Technique for the Joint Selection of Star-forming and Passive Galaxies at 1.4 <\raisebox{-0.5ex}\textasciitilde z <\raisebox{-0.5ex}\textasciitilde 2.5}",
      journal = {\apj},
     keywords = {Cosmology: Observations, Galaxies: Evolution, Galaxies: Formation, Galaxies: High-Redshift, Galaxies: Starburst, Astrophysics},
         year = 2004,
        month = dec,
       volume = {617},
       number = {2},
        pages = {746-764},
          doi = {10.1086/425569},
archivePrefix = {arXiv},
       eprint = {astro-ph/0409041},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2004ApJ...617..746D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{coupon09,
       author = {{Coupon}, J. and {Ilbert}, O. and {Kilbinger}, M. and {McCracken}, H.~J. and {Mellier}, Y. and {Arnouts}, S. and {Bertin}, E. and {Hudelot}, P. and {Schultheis}, M. and {Le F{\`e}vre}, O. and {Le Brun}, V. and {Guzzo}, L. and {Bardelli}, S. and {Zucca}, E. and {Bolzonella}, M. and {Garilli}, B. and {Zamorani}, G. and {Zanichelli}, A. and {Tresse}, L. and {Aussel}, H.},
        title = "{Photometric redshifts for the CFHTLS T0004 deep and wide fields}",
      journal = {\aap},
     keywords = {galaxies: distances and redshifts, cosmology: observations, cosmology: large-scale structure of Universe, Astrophysics},
         year = 2009,
        month = jun,
       volume = {500},
       number = {3},
        pages = {981-998},
          doi = {10.1051/0004-6361/200811413},
archivePrefix = {arXiv},
       eprint = {0811.3326},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009A&A...500..981C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{lee15_ssfr,
       author = {{Lee}, Nicholas and {Sanders}, D.~B. and {Casey}, Caitlin M. and
         {Toft}, Sune and {Scoville}, N.~Z. and {Hung}, Chao-Ling and
         {Le Floc'h}, Emeric and {Ilbert}, Olivier and {Zahid}, H. Jabran and
         {Aussel}, Herv{\'e} and {Capak}, Peter and {Kartaltepe}, Jeyhan S. and
         {Kewley}, Lisa J. and {Li}, Yanxia and {Schawinski}, Kevin and
         {Sheth}, Kartik and {Xiao}, Quanbao},
        title = "{A Turnover in the Galaxy Main Sequence of Star Formation at M $_{*}$ \raisebox{-0.5ex}\textasciitilde {}10$^{10}$ M $_{☉}$ for Redshifts z \&lt; 1.3}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: high-redshift, galaxies: star formation, Astrophysics - Astrophysics of Galaxies},
         year = 2015,
        month = mar,
       volume = {801},
       number = {2},
          eid = {80},
        pages = {80},
          doi = {10.1088/0004-637X/801/2/80},
archivePrefix = {arXiv},
       eprint = {1501.01080},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015ApJ...801...80L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{legrand19_hod,
       author = {{Legrand}, L. and {McCracken}, H.~J. and {Davidzon}, I. and
         {Ilbert}, O. and {Coupon}, J. and {Aghanim}, N. and {Douspis}, M. and
         {Capak}, P.~L. and {Le F{\`e}vre}, O. and {Milvang-Jensen}, B.},
        title = "{The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to z {\ensuremath{\sim}} 5}",
      journal = {\mnras},
     keywords = {methods: statistical, galaxies: evolution, galaxies: haloes, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2019,
        month = jul,
       volume = {486},
       number = {4},
        pages = {5468-5481},
          doi = {10.1093/mnras/stz1198},
archivePrefix = {arXiv},
       eprint = {1810.10557},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.5468L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{karim11_ssfr,
       author = {{Karim}, A. and {Schinnerer}, E. and {Mart{\'\i}nez-Sansigre}, A. and
         {Sargent}, M.~T. and {van der Wel}, A. and {Rix}, H. -W. and
         {Ilbert}, O. and {Smol{\v{c}}i{\'c}}, V. and {Carilli}, C. and
         {Pannella}, M. and {Koekemoer}, A.~M. and {Bell}, E.~F. and
         {Salvato}, M.},
        title = "{The Star Formation History of Mass-selected Galaxies in the COSMOS Field}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: star formation, radio continuum: galaxies, surveys, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2011,
        month = apr,
       volume = {730},
       number = {2},
          eid = {61},
        pages = {61},
          doi = {10.1088/0004-637X/730/2/61},
archivePrefix = {arXiv},
       eprint = {1011.6370},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJ...730...61K},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{novak17_sfrd,
       author = {{Novak}, M. and {Smol{\v{c}}i{\'c}}, V. and {Delhaize}, J. and
         {Delvecchio}, I. and {Zamorani}, G. and {Baran}, N. and {Bondi}, M. and
         {Capak}, P. and {Carilli}, C.~L. and {Ciliegi}, P. and {Civano}, F. and
         {Ilbert}, O. and {Karim}, A. and {Laigle}, C. and {Le F{\`e}vre}, O. and
         {Marchesi}, S. and {McCracken}, H. and {Miettinen}, O. and
         {Salvato}, M. and {Sargent}, M. and {Schinnerer}, E. and {Tasca}, L.},
        title = "{The VLA-COSMOS 3 GHz Large Project: Cosmic star formation history since z   5}",
      journal = {\aap},
     keywords = {galaxies: evolution, galaxies: star formation, cosmology: observations, radio continuum: galaxies, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = jun,
       volume = {602},
          eid = {A5},
        pages = {A5},
          doi = {10.1051/0004-6361/201629436},
archivePrefix = {arXiv},
       eprint = {1703.09724},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017A&A...602A...5N},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{mccracken15_clustering,
       author = {{McCracken}, H.~J. and {Wolk}, M. and {Colombi}, S. and {Kilbinger}, M. and
         {Ilbert}, O. and {Peirani}, S. and {Coupon}, J. and {Dunlop}, J. and
         {Milvang-Jensen}, B. and {Caputi}, K. and {Aussel}, H. and
         {B{\'e}thermin}, M. and {Le F{\`e}vre}, O.},
        title = "{Probing the galaxy-halo connection in UltraVISTA to z {\ensuremath{\sim}} 2}",
      journal = {\mnras},
     keywords = {methods: statistical, galaxies: evolution, galaxies: formation, large-scale structure of Universe, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2015,
        month = may,
       volume = {449},
       number = {1},
        pages = {901-916},
          doi = {10.1093/mnras/stv305},
archivePrefix = {arXiv},
       eprint = {1411.4983},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015MNRAS.449..901M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{cucciati18_highz_cluster,
       author = {{Cucciati}, O. and {Lemaux}, B.~C. and {Zamorani}, G. and
         {Le F{\`e}vre}, O. and {Tasca}, L.~A.~M. and {Hathi}, N.~P. and
         {Lee}, K. -G. and {Bardelli}, S. and {Cassata}, P. and {Garilli}, B. and
         {Le Brun}, V. and {Maccagni}, D. and {Pentericci}, L. and {Thomas}, R. and
         {Vanzella}, E. and {Zucca}, E. and {Lubin}, L.~M. and {Amorin}, R. and
         {Cassar{\`a}}, L.~P. and {Cimatti}, A. and {Talia}, M. and
         {Vergani}, D. and {Koekemoer}, A. and {Pforr}, J. and {Salvato}, M.},
        title = "{The progeny of a cosmic titan: a massive multi-component proto-supercluster in formation at z = 2.45 in VUDS}",
      journal = {\aap},
     keywords = {galaxies: clusters: general, galaxies: high-redshift, cosmology: observations, large-scale structure of Universe, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = nov,
       volume = {619},
          eid = {A49},
        pages = {A49},
          doi = {10.1051/0004-6361/201833655},
archivePrefix = {arXiv},
       eprint = {1806.06073},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018A&A...619A..49C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{capak11_highz_cluster,
       author = {{Capak}, Peter L. and {Riechers}, Dominik and {Scoville}, Nick Z. and
         {Carilli}, Chris and {Cox}, Pierre and {Neri}, Roberto and
         {Robertson}, Brant and {Salvato}, Mara and {Schinnerer}, Eva and
         {Yan}, Lin and {Wilson}, Grant W. and {Yun}, Min and
         {Civano}, Francesca and {Elvis}, Martin and {Karim}, Alexander and
         {Mobasher}, Bahram and {Staguhn}, Johannes G.},
        title = "{A massive protocluster of galaxies at a redshift of z\raisebox{-0.5ex}\textasciitilde5.3}",
      journal = {\nat},
     keywords = {Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2011,
        month = feb,
       volume = {470},
       number = {7333},
        pages = {233-235},
          doi = {10.1038/nature09681},
archivePrefix = {arXiv},
       eprint = {1101.3586},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011Natur.470..233C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{saito20_emitters_COSMOS2015,
       author = {{Saito}, Shun and {de la Torre}, Sylvain and {Ilbert}, Olivier and
         {Dubois}, C{\'e}dric and {Yabe}, Kiyoto and {Coupon}, Jean},
        title = "{The synthetic Emission Line COSMOS catalogue: H{\ensuremath{\alpha}} and [O II] galaxy luminosity functions and counts at 0.3 \&lt; z \&lt; 2.5}",
      journal = {\mnras},
     keywords = {surveys, galaxies: luminosity function, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = mar,
       volume = {494},
       number = {1},
        pages = {199-217},
          doi = {10.1093/mnras/staa727},
archivePrefix = {arXiv},
       eprint = {2003.06394},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.494..199S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{mandelbaum18_weaklensing,
       author = {{Mandelbaum}, Rachel},
        title = "{Weak Lensing for Precision Cosmology}",
      journal = {\araa},
     keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2018,
        month = sep,
       volume = {56},
        pages = {393-433},
          doi = {10.1146/annurev-astro-081817-051928},
archivePrefix = {arXiv},
       eprint = {1710.03235},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ARA&A..56..393M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{masters19_C3R2_2release,
       author = {{Masters}, Daniel C. and {Stern}, Daniel K. and {Cohen}, Judith G. and
         {Capak}, Peter L. and {Stanford}, S. Adam and {Hernitschek}, Nina and
         {Galametz}, Audrey and {Davidzon}, Iary and {Rhodes}, Jason D. and {Sand
        ers}, Dave and {Mobasher}, Bahram and {Castander}, Francisco and
         {Pruett}, Kerianne and {Fotopoulou}, Sotiria},
        title = "{The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Analysis and Data Release 2}",
      journal = {\apj},
     keywords = {astronomical databases, catalogs, cosmology: observations, galaxies: distances and redshifts, surveys, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2019,
        month = jun,
       volume = {877},
       number = {2},
          eid = {81},
        pages = {81},
          doi = {10.3847/1538-4357/ab184d},
archivePrefix = {arXiv},
       eprint = {1904.06394},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...877...81M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Rosani19_catalogue,
       author = {{Rosani}, G. and {Caminha}, G.~B. and {Caputi}, K.~I. and {Deshmukh}, S.},
        title = "{VizieR Online Data Catalog: Bright Lyman-alpha emitters in MUSE/COSMOS field (Rosani+, 2020)}",
      journal = {VizieR Online Data Catalog},
     keywords = {Galaxy catalogs, Redshifts, Optical},
         year = 2019,
        month = nov,
          eid = {J/A+A/633/A159},
        pages = {J/A+A/633/A159},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019yCat..36330159R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Rosani19_paper,
       author = {{Rosani}, G. and {Caminha}, G.~B. and {Caputi}, K.~I. and {Deshmukh}, S.},
        title = "{Bright Lyman-{\ensuremath{\alpha}} emitters among Spitzer SMUVS galaxies in the MUSE/COSMOS field}",
      journal = {\aap},
     keywords = {galaxies: high-redshift, galaxies: star formation, cosmology: observations, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = jan,
       volume = {633},
          eid = {A159},
        pages = {A159},
          doi = {10.1051/0004-6361/201935782},
archivePrefix = {arXiv},
       eprint = {1910.04771},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...633A.159R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Hasinger18_deimos,
       author = {{Hasinger}, G. and {Capak}, P. and {Salvato}, M. and {Barger}, A.~J. and
         {Cowie}, L.~L. and {Faisst}, A. and {Hemmati}, S. and {Kakazu}, Y. and
         {Kartaltepe}, J. and {Masters}, D. and {Mobasher}, B. and
         {Nayyeri}, H. and {Sanders}, D. and {Scoville}, N.~Z. and {Suh}, H. and
         {Steinhardt}, C. and {Yang}, Fengwei},
        title = "{The DEIMOS 10K Spectroscopic Survey Catalog of the COSMOS Field}",
      journal = {\apj},
     keywords = {catalogs, galaxies: distances and redshifts, surveys, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2018,
        month = may,
       volume = {858},
       number = {2},
          eid = {77},
        pages = {77},
          doi = {10.3847/1538-4357/aabacf},
archivePrefix = {arXiv},
       eprint = {1803.09251},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ApJ...858...77H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Sanders_2007,
       author = {{Sanders}, D.~B. and {Salvato}, M. and {Aussel}, H. and {Ilbert}, O. and
         {Scoville}, N. and {Surace}, J.~A. and {Frayer}, D.~T. and {Sheth}, K. and
         {Helou}, G. and {Brooke}, T. and {Bhattacharya}, B. and {Yan}, L. and
         {Kartaltepe}, J.~S. and {Barnes}, J.~E. and {Blain}, A.~W. and
         {Calzetti}, D. and {Capak}, P. and {Carilli}, C. and {Carollo}, C.~M. and
         {Comastri}, A. and {Daddi}, E. and {Ellis}, R.~S. and {Elvis}, M. and
         {Fall}, S.~M. and {Franceschini}, A. and {Giavalisco}, M. and
         {Hasinger}, G. and {Impey}, C. and {Koekemoer}, A. and
         {Le F{\`e}vre}, O. and {Lilly}, S. and {Liu}, M.~C. and
         {McCracken}, H.~J. and {Mobasher}, B. and {Renzini}, A. and {Rich}, M. and
         {Schinnerer}, E. and {Shopbell}, P.~L. and {Taniguchi}, Y. and
         {Thompson}, D.~J. and {Urry}, C.~M. and {Williams}, J.~P.},
        title = "{S-COSMOS: The Spitzer Legacy Survey of the Hubble Space Telescope ACS 2 deg$^{2}$ COSMOS Field I: Survey Strategy and First Analysis}",
      journal = {\apjs},
     keywords = {Cosmology: Observations, Galaxies: Evolution, Galaxies: Formation, Infrared: Galaxies, Cosmology: Large-Scale Structure of Universe, Surveys, Astrophysics},
         year = 2007,
        month = sep,
       volume = {172},
       number = {1},
        pages = {86-98},
          doi = {10.1086/517885},
archivePrefix = {arXiv},
       eprint = {astro-ph/0701318},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007ApJS..172...86S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Kashino19_FMOS-COSMOS,
       author = {{Kashino}, Daichi and {Silverman}, John D. and {Sanders}, David and
         {Kartaltepe}, Jeyhan and {Daddi}, Emanuele and {Renzini}, Alvio and
         {Rodighiero}, Giulia and {Puglisi}, Annagrazia and
         {Valentino}, Francesco and {Juneau}, St{\'e}phanie and
         {Arimoto}, Nobuo and {Nagao}, Tohru and {Ilbert}, Olivier and
         {Le F{\`e}vre}, Olivier and {Koekemoer}, Anton M.},
        title = "{The FMOS-COSMOS Survey of Star-forming Galaxies at z {\ensuremath{\sim}} 1.6. VI. Redshift and Emission-line Catalog and Basic Properties of Star-forming Galaxies}",
      journal = {\apjs},
     keywords = {catalogs, galaxies: evolution, galaxies: ISM, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = mar,
       volume = {241},
       number = {1},
          eid = {10},
        pages = {10},
          doi = {10.3847/1538-4365/ab06c4},
archivePrefix = {arXiv},
       eprint = {1812.01529},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJS..241...10K},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{Bacon2010_muse,
       author = {{Bacon}, R. and {Accardo}, M. and {Adjali}, L. and {Anwand}, H. and
         {Bauer}, S. and {Biswas}, I. and {Blaizot}, J. and {Boudon}, D. and
         {Brau-Nogue}, S. and {Brinchmann}, J. and {Caillier}, P. and
         {Capoani}, L. and {Carollo}, C.~M. and {Contini}, T. and {Couderc}, P. and
         {Daguis{\'e}}, E. and {Deiries}, S. and {Delabre}, B. and
         {Dreizler}, S. and {Dubois}, J. and {Dupieux}, M. and {Dupuy}, C. and
         {Emsellem}, E. and {Fechner}, T. and {Fleischmann}, A. and
         {Fran{\c{c}}ois}, M. and {Gallou}, G. and {Gharsa}, T. and
         {Glindemann}, A. and {Gojak}, D. and {Guiderdoni}, B. and
         {Hansali}, G. and {Hahn}, T. and {Jarno}, A. and {Kelz}, A. and
         {Koehler}, C. and {Kosmalski}, J. and {Laurent}, F. and {Le Floch}, M. and
         {Lilly}, S.~J. and {Lizon}, J. -L. and {Loupias}, M. and
         {Manescau}, A. and {Monstein}, C. and {Nicklas}, H. and
         {Olaya}, J. -C. and {Pares}, L. and {Pasquini}, L. and
         {P{\'e}contal-Rousset}, A. and {Pell{\'o}}, R. and {Petit}, C. and
         {Popow}, E. and {Reiss}, R. and {Remillieux}, A. and {Renault}, E. and
         {Roth}, M. and {Rupprecht}, G. and {Serre}, D. and {Schaye}, J. and
         {Soucail}, G. and {Steinmetz}, M. and {Streicher}, O. and {Stuik}, R. and
         {Valentin}, H., and {Vernet}, J. and {Weilbacher}, P. and
         {Wisotzki}, L. and {Yerle}, N.},
        title = "{The MUSE second-generation VLT instrument}",
    booktitle = {Ground-based and Airborne Instrumentation for Astronomy III},
         year = 2010,
       series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
       volume = {7735},
        month = jul,
          eid = {773508},
        pages = {773508},
          doi = {10.1117/12.856027},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010SPIE.7735E..08B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{kohonen82_som,
   author = {{Kohonen}, T.},
    title = "{elf-organized formation of topologically correct feature maps}",
  journal = {Biol. Cybern.},
     year = 1982,
   volume = 43,
    pages = {59-69},
}


@ARTICLE{lilly07_zcosmos,
   author = {{Lilly}, S.~J. and {Le F{\`e}vre}, O. and {Renzini}, A. and 
	{Zamorani}, G. and {Scodeggio}, M. and {Contini}, T. and {Carollo}, C.~M. and 
	{Hasinger}, G. and {Kneib}, J.-P. and {Iovino}, A. and {Le Brun}, V. and 
	{Maier}, C. and {Mainieri}, V. and {Mignoli}, M. and {Silverman}, J. and 
	{Tasca}, L.~A.~M. and {Bolzonella}, M. and {Bongiorno}, A. and 
	{Bottini}, D. and {Capak}, P. and {Caputi}, K. and {Cimatti}, A. and 
	{Cucciati}, O. and {Daddi}, E. and {Feldmann}, R. and {Franzetti}, P. and 
	{Garilli}, B. and {Guzzo}, L. and {Ilbert}, O. and {Kampczyk}, P. and 
	{Kovac},, K. and {Lamareille}, F. and {Leauthaud}, A. and {Le Borgne}, J.-F. and 
	{McCracken}, H.~J. and {Marinoni}, C. and {Pello}, R. and {Ricciardelli}, E. and 
	{Scarlata}, C. and {Vergani}, D. and {Sanders}, D.~B. and {Schinnerer}, E. and 
	{Scoville}, N. and {Taniguchi}, Y. and {Arnouts}, S. and {Aussel}, H. and 
	{Bardelli}, S. and {Brusa}, M. and {Cappi}, A. and {Ciliegi}, P. and 
	{Finoguenov}, A. and {Foucaud}, S. and {Franceschini}, A. and 
	{Halliday}, C. and {Impey}, C. and {Knobel}, C. and {Koekemoer}, A. and 
	{Kurk}, J. and {Maccagni}, D. and {Maddox}, S. and {Marano}, B. and 
	{Marconi}, G. and {Meneux}, B. and {Mobasher}, B. and {Moreau}, C. and 
	{Peacock}, J.~A. and {Porciani}, C. and {Pozzetti}, L. and {Scaramella}, R. and 
	{Schiminovich}, D. and {Shopbell}, P. and {Smail}, I. and {Thompson}, D. and 
	{Tresse}, L. and {Vettolani}, G. and {Zanichelli}, A. and {Zucca}, E.
	},
    title = "{zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 $\lt$ z $\lt$ 3 in the COSMOS Field}",
  journal = {\apjs},
   eprint = {astro-ph/0612291},
 keywords = {Cosmology: Observations, Galaxies: Active, Galaxies: Distances and Redshifts, Galaxies: Evolution, Cosmology: Large-Scale Structure of Universe, Galaxies: Quasars: General, Surveys},
     year = 2007,
    month = sep,
   volume = 172,
    pages = {70-85},
      doi = {10.1086/516589},
   adsurl = {http://cdsads.u-strasbg.fr/abs/2007ApJS..172...70L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{lefevre15,
   author = {{Le F{\`e}vre}, O. and {Tasca}, L.~A.~M. and {Cassata}, P. and 
	{Garilli}, B. and {Le Brun}, V. and {Maccagni}, D. and {Pentericci}, L. and 
	{Thomas}, R. and {Vanzella}, E. and {Zamorani}, G. and {Zucca}, E. and 
	{Amorin}, R. and {Bardelli}, S. and {Capak}, P. and {Cassar{\`a}}, L. and 
	{Castellano}, M. and {Cimatti}, A. and {Cuby}, J.~G. and {Cucciati}, O. and 
	{de la Torre}, S. and {Durkalec}, A. and {Fontana}, A. and {Giavalisco}, M. and 
	{Grazian}, A. and {Hathi}, N.~P. and {Ilbert}, O. and {Lemaux}, B.~C. and 
	{Moreau}, C. and {Paltani}, S. and {Ribeiro}, B. and {Salvato}, M. and 
	{Schaerer}, D. and {Scodeggio}, M. and {Sommariva}, V. and {Talia}, M. and 
	{Taniguchi}, Y. and {Tresse}, L. and {Vergani}, D. and {Wang}, P.~W. and 
	{Charlot}, S. and {Contini}, T. and {Fotopoulou}, S. and {L{\'o}pez-Sanjuan}, C. and 
	{Mellier}, Y. and {Scoville}, N.},
    title = "{The VIMOS Ultra-Deep Survey: \~{}10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 $\lt$ z {\sime} 6}",
  journal = {\aap},
archivePrefix = "arXiv",
   eprint = {1403.3938},
 keywords = {galaxies: evolution, galaxies: high-redshift, cosmology: observations, large-scale structure of Universe, surveys, galaxies: formation},
     year = 2015,
    month = apr,
   volume = 576,
      eid = {A79},
    pages = {A79},
      doi = {10.1051/0004-6361/201423829},
   adsurl = {http://cdsads.u-strasbg.fr/abs/2015A%26A...576A..79L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{lefevre03,
       author = {{Le F{\`e}vre}, Oliver and {Saisse}, Michel and {Mancini}, Dario and
         {Brau-Nogue}, Sylvie and {Caputi}, Oreste and {Castinel}, Louis and
         {D'Odorico}, Sandro and {Garilli}, Bianca and {Kissler-Patig}, Markus and
         {Lucuix}, Christian and {Mancini}, Guido and {Pauget}, Alain and
         {Sciarretta}, Giovanni and {Scodeggio}, Marco and {Tresse}, Laurence and
         {Vettolani}, Gianpaolo},
        title = "{Commissioning and performances of the VLT-VIMOS instrument}",
    booktitle = {Instrument Design and Performance for Optical/Infrared Ground-based Telescopes},
         year = 2003,
       editor = {{Iye}, Masanori and {Moorwood}, Alan F.~M.},
       series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
       volume = {4841},
        month = mar,
        pages = {1670-1681},
          doi = {10.1117/12.460959},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2003SPIE.4841.1670L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{vanderwel16_legac,
       author = {{van der Wel}, A. and {Noeske}, K. and {Bezanson}, R. and
         {Pacifici}, C. and {Gallazzi}, A. and {Franx}, M. and
         {Mu{\~n}oz-Mateos}, J.~C. and {Bell}, E.~F. and {Brammer}, G. and
         {Charlot}, S. and {Chauk{\'e}}, P. and {Labb{\'e}}, I. and
         {Maseda}, M.~V. and {Muzzin}, A. and {Rix}, H. -W. and {Sobral}, D. and
         {van de Sande}, J. and {van Dokkum}, P.~G. and {Wild}, V. and
         {Wolf}, C.},
        title = "{The VLT LEGA-C Spectroscopic Survey: The Physics of Galaxies at a Lookback Time of 7 Gyr}",
      journal = {\apjs},
     keywords = {galaxies: evolution, galaxies: fundamental parameters, galaxies: general, galaxies: stellar content, surveys, Astrophysics - Astrophysics of Galaxies},
         year = "2016",
        month = "Apr",
       volume = {223},
       number = {2},
          eid = {29},
        pages = {29},
          doi = {10.3847/0067-0049/223/2/29},
archivePrefix = {arXiv},
       eprint = {1603.05479},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016ApJS..223...29V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{scoville17_ALMA,
       author = {{Scoville}, N. and {Lee}, N. and {Vanden Bout}, P. and
         {Diaz-Santos}, T. and {Sanders}, D. and {Darvish}, B. and
         {Bongiorno}, A. and {Casey}, C.~M. and {Murchikova}, L. and {Koda}, J. and
         {Capak}, P. and {Vlahakis}, Catherine and {Ilbert}, O. and {Sheth}, K. and
         {Morokuma-Matsui}, K. and {Ivison}, R.~J. and {Aussel}, H. and
         {Laigle}, C. and {McCracken}, H.~J. and {Armus}, L. and {Pope}, A. and
         {Toft}, S. and {Masters}, D.},
        title = "{Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift}",
      journal = {\apj},
     keywords = {accretion, accretion disks, evolution, galaxies: ISM, galaxies: starburst, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = mar,
       volume = {837},
       number = {2},
          eid = {150},
        pages = {150},
          doi = {10.3847/1538-4357/aa61a0},
archivePrefix = {arXiv},
       eprint = {1702.04729},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017ApJ...837..150S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{lefevre19_alpine,
       author = {{Le F{\`e}vre}, O. and {B{\'e}thermin}, M. and {Faisst}, A. and
         {Jones}, G. and {Capak}, P. and {Cassata}, P. and {Silverman}, J.~D. and
         {Schaerer}, D. and {Yan}, L. and {the ALPINE team}},
        title = "{The ALPINE-ALMA [CII] survey: Survey strategy, observations and sample properties of 118 star-forming galaxies at $4&lt;z&lt;6$}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = oct,
          eid = {arXiv:1910.09517},
        pages = {arXiv:1910.09517},
archivePrefix = {arXiv},
       eprint = {1910.09517},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019arXiv191009517L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Thorne2021,
       author = {{Thorne}, Jessica E. and {Robotham}, Aaron S.~G. and {Davies}, Luke J.~M. and {Bellstedt}, Sabine and {Driver}, Simon P. and {Bravo}, Mat{\'\i}as and {Bremer}, Malcolm N. and {Holwerda}, Benne W. and {Hopkins}, Andrew M. and {Lagos}, Claudia del P. and {Phillipps}, Steven and {Siudek}, Malgorzata and {Taylor}, Edward N. and {Wright}, Angus H.},
        title = "{Deep Extragalactic VIsible Legacy Survey (DEVILS): SED fitting in the D10-COSMOS field and the evolution of the stellar mass function and SFR-M$_{{\ensuremath{\star}}}$ relation}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: general, galaxies: star formation, galaxies: stellar content, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = jul,
       volume = {505},
       number = {1},
        pages = {540-567},
          doi = {10.1093/mnras/stab1294},
archivePrefix = {arXiv},
       eprint = {2011.13605},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.505..540T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Kauffmann2022,
       author = {{Kauffmann}, O.~B. and {Ilbert}, O. and {Weaver}, J.~R. and {McCracken}, H.~J. and {Milvang-Jensen}, B. and {Brammer}, G. and {Davidzon}, I. and {Le F{\`e}vre}, O. and {Liu}, D. and {Mobasher}, B. and {Moneti}, A. and {Shuntov}, M. and {Toft}, S. and {Casey}, C.~M. and {Dunlop}, J.~S. and {Kartaltepe}, J.~S. and {Koekemoer}, A.~M. and {Sanders}, D.~B. and {Tresse}, L.},
        title = "{COSMOS2020: UV selected galaxies at $z\geq7.5$}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = jul,
          eid = {arXiv:2207.11740},
        pages = {arXiv:2207.11740},
archivePrefix = {arXiv},
       eprint = {2207.11740},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220711740K},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{foster-schreiber09_sins,
       author = {{F{\"o}rster Schreiber}, N.~M. and {Genzel}, R. and {Bouch{\'e}}, N. and
         {Cresci}, G. and {Davies}, R. and {Buschkamp}, P. and {Shapiro}, K. and
         {Tacconi}, L.~J. and {Hicks}, E.~K.~S. and {Genel}, S. and
         {Shapley}, A.~E. and {Erb}, D.~K. and {Steidel}, C.~C. and {Lutz}, D. and
         {Eisenhauer}, F. and {Gillessen}, S. and {Sternberg}, A. and
         {Renzini}, A. and {Cimatti}, A. and {Daddi}, E. and {Kurk}, J. and
         {Lilly}, S. and {Kong}, X. and {Lehnert}, M.~D. and {Nesvadba}, N. and
         {Verma}, A. and {McCracken}, H. and {Arimoto}, N. and {Mignoli}, M. and
         {Onodera}, M.},
        title = "{The SINS Survey: SINFONI Integral Field Spectroscopy of z \raisebox{-0.5ex}\textasciitilde 2 Star-forming Galaxies}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: high-redshift, galaxies: kinematics and dynamics, infrared: galaxies, Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - Galaxy Astrophysics},
         year = 2009,
        month = dec,
       volume = {706},
       number = {2},
        pages = {1364-1428},
          doi = {10.1088/0004-637X/706/2/1364},
archivePrefix = {arXiv},
       eprint = {0903.1872},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009ApJ...706.1364F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{taniguchi15_medium_bands,
       author = {{Taniguchi}, Yoshiaki and {Kajisawa}, Masaru and
         {Kobayashi}, Masakazu A.~R. and {Shioya}, Yasuhiro and {Nagao}, Tohru and
         {Capak}, Peter L. and {Aussel}, Herve and {Ichikawa}, Akie and
         {Murayama}, Takashi and {Scoville}, Nick Z. and {Ilbert}, Olivier and
         {Salvato}, Mara and {Sanders}, David B.~B. and {Mobasher}, Bahram and
         {Miyazaki}, Satoshi and {Komiyama}, Yutaka and {Le F{\`e}vre}, Olivier and
         {Tasca}, Lidia and {Lilly}, Simon and {Carollo}, Marcella and
         {Renzini}, Alvio and {Rich}, Michael and {Schinnerer}, Eva and
         {Kaifu}, Norio and {Karoji}, Hiroshi and {Arimoto}, Nobuo and
         {Okamura}, Sadanori and {Ohta}, Kouji and {Shimasaku}, Kazuhiro and
         {Hayashino}, Tomoki},
        title = "{The Subaru COSMOS 20: Subaru optical imaging of the HST COSMOS field with 20 filters*}",
      journal = {\pasj},
     keywords = {methods: observational, surveys, techniques: photometric, Astrophysics - Astrophysics of Galaxies},
         year = 2015,
        month = dec,
       volume = {67},
       number = {6},
          eid = {104},
        pages = {104},
          doi = {10.1093/pasj/psv106},
archivePrefix = {arXiv},
       eprint = {1510.00550},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015PASJ...67..104T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{miyazaki12_hsc_camera,
       author = {{Miyazaki}, Satoshi and {Komiyama}, Yutaka and {Nakaya}, Hidehiko and
         {Kamata}, Yukiko and {Doi}, Yoshi and {Hamana}, Takashi and
         {Karoji}, Hiroshi and {Furusawa}, Hisanori and {Kawanomoto}, Satoshi and
         {Morokuma}, Tomoki and {Ishizuka}, Yuki and {Nariai}, Kyoji and
         {Tanaka}, Yoko and {Uraguchi}, Fumihiro and {Utsumi}, Yousuke and
         {Obuchi}, Yoshiyuki and {Okura}, Yuki and {Oguri}, Masamune and
         {Takata}, Tadafumi and {Tomono}, Daigo and {Kurakami}, Tomio and
         {Namikawa}, Kazuhito and {Usuda}, Tomonori and {Yamanoi}, Hitomi and
         {Terai}, Tsuyoshi and {Uekiyo}, Hatsue and {Yamada}, Yoshihiko and
         {Koike}, Michitaro and {Aihara}, Hiro and {Fujimori}, Yuki and
         {Mineo}, Sogo and {Miyatake}, Hironao and {Yasuda}, Naoki and
         {Nishizawa}, Jun and {Saito}, Tomoki and {Tanaka}, Manobu and
         {Uchida}, Tomohisa and {Katayama}, Nobu and {Wang}, Shiang-Yu and
         {Chen}, Hsin-Yo and {Lupton}, Robert and {Loomis}, Craig and
         {Bickerton}, Steve and {Price}, Paul and {Gunn}, Jim and
         {Suzuki}, Hisanori and {Miyazaki}, Yasuhito and {Muramatsu}, Masaharu and
         {Yamamoto}, Koei and {Endo}, Makoto and {Ezaki}, Yutaka and
         {Itoh}, Noboru and {Miwa}, Yoshinori and {Yokota}, Hideo and
         {Matsuda}, Toru and {Ebinuma}, Ryuichi and {Takeshi}, Kunio},
        title = "{Hyper Suprime-Cam}",
    booktitle = {\procspie},
         year = 2012,
       series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
       volume = {8446},
        month = sep,
          eid = {84460Z},
        pages = {84460Z},
          doi = {10.1117/12.926844},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012SPIE.8446E..0ZM},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{hildebrandt12_cfhtlens,
       author = {{Hildebrandt}, H. and {Erben}, T. and {Kuijken}, K. and
         {van Waerbeke}, L. and {Heymans}, C. and {Coupon}, J. and
         {Benjamin}, J. and {Bonnett}, C. and {Fu}, L. and {Hoekstra}, H. and
         {Kitching}, T.~D. and {Mellier}, Y. and {Miller}, L. and {Veland
        er}, M. and {Hudson}, M.~J. and {Rowe}, B.~T.~P. and {Schrabback}, T. and
         {Semboloni}, E. and {Ben{\'\i}tez}, N.},
        title = "{CFHTLenS: improving the quality of photometric redshifts with precision photometry}",
      journal = {\mnras},
     keywords = {galaxies: abundances, galaxies: high-redshift, galaxies: photometry, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2012,
        month = apr,
       volume = {421},
       number = {3},
        pages = {2355-2367},
          doi = {10.1111/j.1365-2966.2012.20468.x},
archivePrefix = {arXiv},
       eprint = {1111.4434},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012MNRAS.421.2355H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{laidler07_tfit,
       author = {{Laidler}, Victoria G. and {Papovich}, Casey and {Grogin}, Norman A. and
         {Idzi}, Rafal and {Dickinson}, Mark and {Ferguson}, Henry C. and
         {Hilbert}, Bryan and {Clubb}, Kelsey and {Ravindranath}, Swara},
        title = "{TFIT: A Photometry Package Using Prior Information for Mixed-Resolution Data Sets}",
      journal = {\pasp},
     keywords = {Data Analysis and Techniques},
         year = 2007,
        month = nov,
       volume = {119},
       number = {861},
        pages = {1325-1344},
          doi = {10.1086/523898},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007PASP..119.1325L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{desantis07_convphot,
       author = {{De Santis}, C. and {Grazian}, A. and {Fontana}, A. and {Santini}, P.},
        title = "{ConvPhot: A profile-matching algorithm for precision photometry}",
      journal = {\na},
     keywords = {Astrophysics},
         year = 2007,
        month = feb,
       volume = {12},
       number = {4},
        pages = {271-288},
          doi = {10.1016/j.newast.2006.10.004},
archivePrefix = {arXiv},
       eprint = {astro-ph/0701232},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007NewA...12..271D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{merlin16_tphot,
       author = {{Merlin}, E. and {Bourne}, N. and {Castellano}, M. and
         {Ferguson}, H.~C. and {Wang}, T. and {Derriere}, S. and
         {Dunlop}, J.~S. and {Elbaz}, D. and {Fontana}, A.},
        title = "{T-PHOT version 2.0: Improved algorithms for background subtraction, local convolution, kernel registration, and new options}",
      journal = {\aap},
     keywords = {methods: data analysis, techniques: photometric, galaxies: photometry, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = nov,
       volume = {595},
          eid = {A97},
        pages = {A97},
          doi = {10.1051/0004-6361/201628751},
archivePrefix = {arXiv},
       eprint = {1609.00146},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016A&A...595A..97M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Dahlen13_candels,
       author = {{Dahlen}, Tomas and {Mobasher}, Bahram and {Faber}, Sandra M. and
         {Ferguson}, Henry C. and {Barro}, Guillermo and
         {Finkelstein}, Steven L. and {Finlator}, Kristian and
         {Fontana}, Adriano and {Gruetzbauch}, Ruth and {Johnson}, Seth and
         {Pforr}, Janine and {Salvato}, Mara and {Wiklind}, Tommy and
         {Wuyts}, Stijn and {Acquaviva}, Viviana and {Dickinson}, Mark E. and
         {Guo}, Yicheng and {Huang}, Jiasheng and {Huang}, Kuang-Han and
         {Newman}, Jeffrey A. and {Bell}, Eric F. and
         {Conselice}, Christopher J. and {Galametz}, Audrey and {Gawiser}, Eric and
         {Giavalisco}, Mauro and {Grogin}, Norman A. and {Hathi}, Nimish and
         {Kocevski}, Dale and {Koekemoer}, Anton M. and {Koo}, David C. and
         {Lee}, Kyoung-Soo and {McGrath}, Elizabeth J. and {Papovich}, Casey and
         {Peth}, Michael and {Ryan}, Russell and {Somerville}, Rachel and
         {Weiner}, Benjamin and {Wilson}, Grant},
        title = "{A Critical Assessment of Photometric Redshift Methods: A CANDELS Investigation}",
      journal = {\apj},
     keywords = {galaxies: distances and redshifts, galaxies: high-redshift, galaxies: photometry, surveys, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = oct,
       volume = {775},
       number = {2},
          eid = {93},
        pages = {93},
          doi = {10.1088/0004-637X/775/2/93},
archivePrefix = {arXiv},
       eprint = {1308.5353},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJ...775...93D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Nyland17_servs_tractor,
       author = {{Nyland}, Kristina and {Lacy}, Mark and {Sajina}, Anna and
         {Pforr}, Janine and {Farrah}, Duncan and {Wilson}, Gillian and
         {Surace}, Jason and {H{\"a}u{\ss}ler}, Boris and {Vaccari}, Mattia and
         {Jarvis}, Matt},
        title = "{An Application of Multi-band Forced Photometry to One Square Degree of SERVS: Accurate Photometric Redshifts and Implications for Future Science}",
      journal = {\apjs},
     keywords = {catalogs, Galaxies: evolution, methods: data analysis, surveys, techniques: image processing, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = may,
       volume = {230},
       number = {1},
          eid = {9},
        pages = {9},
          doi = {10.3847/1538-4365/aa6fed},
archivePrefix = {arXiv},
       eprint = {1704.01582},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017ApJS..230....9N},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{dejong15_kids,
       author = {{de Jong}, Jelte T.~A. and {Verdoes Kleijn}, Gijs A. and
         {Boxhoorn}, Danny R. and {Buddelmeijer}, Hugo and
         {Capaccioli}, Massimo and {Getman}, Fedor and {Grado}, Aniello and
         {Helmich}, Ewout and {Huang}, Zhuoyi and {Irisarri}, Nancy and
         {Kuijken}, Konrad and {La Barbera}, Francesco and {McFarland}, John P. and
         {Napolitano}, Nicola R. and {Radovich}, Mario and {Sikkema}, Gert and
         {Valentijn}, Edwin A. and {Begeman}, Kor G. and {Brescia}, Massimo and
         {Cavuoti}, Stefano and {Choi}, Ami and {Cordes}, Oliver-Mark and
         {Covone}, Giovanni and {Dall'Ora}, Massimo and {Hildebrandt}, Hendrik and
         {Longo}, Giuseppe and {Nakajima}, Reiko and {Paolillo}, Maurizio and
         {Puddu}, Emanuella and {Rifatto}, Agatino and {Tortora}, Crescenzo and
         {van Uitert}, Edo and {Buddendiek}, Axel and
         {Harnois-D{\'e}raps}, Joachim and {Erben}, Thomas and
         {Eriksen}, Martin B. and {Heymans}, Catherine and {Hoekstra}, Henk and
         {Joachimi}, Benjamin and {Kitching}, Thomas D. and {Klaes}, Dominik and
         {Koopmans}, L{\'e}on V.~E. and {K{\"o}hlinger}, Fabian and
         {Roy}, Nivya and {Sif{\'o}n}, Crist{\'o}bal and {Schneider}, Peter and
         {Sutherland}, Will J. and {Viola}, Massimo and {Vriend}, Willem-Jan},
        title = "{The first and second data releases of the Kilo-Degree Survey}",
      journal = {\aap},
     keywords = {methods: observational, surveys, galaxies: general, large-scale structure of Universe, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2015,
        month = oct,
       volume = {582},
          eid = {A62},
        pages = {A62},
          doi = {10.1051/0004-6361/201526601},
archivePrefix = {arXiv},
       eprint = {1507.00742},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015A&A...582A..62D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{DES05,
       author = {{The Dark Energy Survey Collaboration}},
        title = "{The Dark Energy Survey}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics},
         year = 2005,
        month = oct,
          eid = {astro-ph/0510346},
        pages = {astro-ph/0510346},
archivePrefix = {arXiv},
       eprint = {astro-ph/0510346},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2005astro.ph.10346T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{aihara18_ssp,
       author = {{Aihara}, Hiroaki and {Arimoto}, Nobuo and {Armstrong}, Robert and
         {Arnouts}, St{\'e}phane and {Bahcall}, Neta A. and {Bickerton}, Steven and
         {Bosch}, James and {Bundy}, Kevin and {Capak}, Peter L. and
         {Chan}, James H.~H. and {Chiba}, Masashi and {Coupon}, Jean and
         {Egami}, Eiichi and {Enoki}, Motohiro and {Finet}, Francois and
         {Fujimori}, Hiroki and {Fujimoto}, Seiji and {Furusawa}, Hisanori and
         {Furusawa}, Junko and {Goto}, Tomotsugu and {Goulding}, Andy and
         {Greco}, Johnny P. and {Greene}, Jenny E. and {Gunn}, James E. and
         {Hamana}, Takashi and {Harikane}, Yuichi and {Hashimoto}, Yasuhiro and
         {Hattori}, Takashi and {Hayashi}, Masao and {Hayashi}, Yusuke and
         {He{\l}miniak}, Krzysztof G. and {Higuchi}, Ryo and {Hikage}, Chiaki and
         {Ho}, Paul T.~P. and {Hsieh}, Bau-Ching and {Huang}, Kuiyun and
         {Huang}, Song and {Ikeda}, Hiroyuki and {Imanishi}, Masatoshi and
         {Inoue}, Akio K. and {Iwasawa}, Kazushi and {Iwata}, Ikuru and
         {Jaelani}, Anton T. and {Jian}, Hung-Yu and {Kamata}, Yukiko and
         {Karoji}, Hiroshi and {Kashikawa}, Nobunari and {Katayama}, Nobuhiko and
         {Kawanomoto}, Satoshi and {Kayo}, Issha and {Koda}, Jin and
         {Koike}, Michitaro and {Kojima}, Takashi and {Komiyama}, Yutaka and
         {Konno}, Akira and {Koshida}, Shintaro and {Koyama}, Yusei and
         {Kusakabe}, Haruka and {Leauthaud}, Alexie and {Lee}, Chien-Hsiu and
         {Lin}, Lihwai and {Lin}, Yen-Ting and {Lupton}, Robert H. and {Mand
        elbaum}, Rachel and {Matsuoka}, Yoshiki and {Medezinski}, Elinor and
         {Mineo}, Sogo and {Miyama}, Shoken and {Miyatake}, Hironao and
         {Miyazaki}, Satoshi and {Momose}, Rieko and {More}, Anupreeta and
         {More}, Surhud and {Moritani}, Yuki and {Moriya}, Takashi J. and
         {Morokuma}, Tomoki and {Mukae}, Shiro and {Murata}, Ryoma and
         {Murayama}, Hitoshi and {Nagao}, Tohru and {Nakata}, Fumiaki and
         {Niida}, Mana and {Niikura}, Hiroko and {Nishizawa}, Atsushi J. and
         {Obuchi}, Yoshiyuki and {Oguri}, Masamune and {Oishi}, Yukie and
         {Okabe}, Nobuhiro and {Okamoto}, Sakurako and {Okura}, Yuki and
         {Ono}, Yoshiaki and {Onodera}, Masato and {Onoue}, Masafusa and
         {Osato}, Ken and {Ouchi}, Masami and {Price}, Paul A. and
         {Pyo}, Tae-Soo and {Sako}, Masao and {Sawicki}, Marcin and
         {Shibuya}, Takatoshi and {Shimasaku}, Kazuhiro and {Shimono}, Atsushi and
         {Shirasaki}, Masato and {Silverman}, John D. and {Simet}, Melanie and
         {Speagle}, Joshua and {Spergel}, David N. and {Strauss}, Michael A. and
         {Sugahara}, Yuma and {Sugiyama}, Naoshi and {Suto}, Yasushi and
         {Suyu}, Sherry H. and {Suzuki}, Nao and {Tait}, Philip J. and
         {Takada}, Masahiro and {Takata}, Tadafumi and {Tamura}, Naoyuki and
         {Tanaka}, Manobu M. and {Tanaka}, Masaomi and {Tanaka}, Masayuki and
         {Tanaka}, Yoko and {Terai}, Tsuyoshi and {Terashima}, Yuichi and
         {Toba}, Yoshiki and {Tominaga}, Nozomu and {Toshikawa}, Jun and
         {Turner}, Edwin L. and {Uchida}, Tomohisa and {Uchiyama}, Hisakazu and
         {Umetsu}, Keiichi and {Uraguchi}, Fumihiro and {Urata}, Yuji and
         {Usuda}, Tomonori and {Utsumi}, Yousuke and {Wang}, Shiang-Yu and
         {Wang}, Wei-Hao and {Wong}, Kenneth C. and {Yabe}, Kiyoto and
         {Yamada}, Yoshihiko and {Yamanoi}, Hitomi and {Yasuda}, Naoki and
         {Yeh}, Sherry and {Yonehara}, Atsunori and {Yuma}, Suraphong},
        title = "{The Hyper Suprime-Cam SSP Survey: Overview and survey design}",
      journal = {\pasj},
     keywords = {cosmology: observations, galaxies: general, large-scale structure of universe, surveys, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2018,
        month = jan,
       volume = {70},
          eid = {S4},
        pages = {S4},
          doi = {10.1093/pasj/psx066},
archivePrefix = {arXiv},
       eprint = {1704.05858},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018PASJ...70S...4A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{caputi15_highz_mass,
       author = {{Caputi}, K.~I. and {Ilbert}, O. and {Laigle}, C. and
         {McCracken}, H.~J. and {Le F{\`e}vre}, O. and {Fynbo}, J. and
         {Milvang-Jensen}, B. and {Capak}, P. and {Salvato}, M. and
         {Taniguchi}, Y.},
        title = "{Spitzer Bright, UltraVISTA Faint Sources in COSMOS: The Contribution to the Overall Population of Massive Galaxies at z = 3-7}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: high-redshift, infrared: galaxies, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2015,
        month = sep,
       volume = {810},
       number = {1},
          eid = {73},
        pages = {73},
          doi = {10.1088/0004-637X/810/1/73},
archivePrefix = {arXiv},
       eprint = {1505.05721},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015ApJ...810...73C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{comparat15,
       author = {{Comparat}, Johan and {Richard}, Johan and {Kneib}, Jean-Paul and
         {Ilbert}, Olivier and {Gonzalez-Perez}, Violeta and {Tresse}, Laurence and
         {Zoubian}, Julien and {Arnouts}, Stephane and {Brownstein}, Joel R. and
         {Baugh}, Carlton and {Delubac}, Timothee and {Ealet}, Anne and
         {Escoffier}, Stephanie and {Ge}, Jian and {Jullo}, Eric and
         {Lacey}, Cedric and {Ross}, Nicholas P. and {Schlegel}, David and
         {Schneider}, Donald P. and {Steele}, Oliver and {Tasca}, Lidia and
         {Yeche}, Christophe and {Lesser}, Michael and {Jiang}, Zhaoji and
         {Jing}, Yipeng and {Fan}, Zhou and {Fan}, Xiaohui and {Ma}, Jun and
         {Nie}, Jundan and {Wang}, Jiali and {Wu}, Zhenyu and {Zhang}, Tianmeng and
         {Zhou}, Xu and {Zhou}, Zhimin and {Zou}, Hu},
        title = "{The 0.1 <z < 1.65 evolution of the bright end of the [O ii] luminosity function}",
      journal = {\aap},
     keywords = {catalogs, surveys, galaxies: luminosity function, mass function, cosmology: observations, galaxies: statistics, galaxies: evolution, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2015,
        month = mar,
       volume = {575},
          eid = {A40},
        pages = {A40},
          doi = {10.1051/0004-6361/201424767},
archivePrefix = {arXiv},
       eprint = {1408.1523},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015A&A...575A..40C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{lefevre13_VVDS_final,
       author = {{Le F{\`e}vre}, O. and {Cassata}, P. and {Cucciati}, O. and
         {Garilli}, B. and {Ilbert}, O. and {Le Brun}, V. and {Maccagni}, D. and
         {Moreau}, C. and {Scodeggio}, M. and {Tresse}, L. and {Zamorani}, G. and
         {Adami}, C. and {Arnouts}, S. and {Bardelli}, S. and {Bolzonella}, M. and
         {Bondi}, M. and {Bongiorno}, A. and {Bottini}, D. and {Cappi}, A. and
         {Charlot}, S. and {Ciliegi}, P. and {Contini}, T. and
         {de la Torre}, S. and {Foucaud}, S. and {Franzetti}, P. and
         {Gavignaud}, I. and {Guzzo}, L. and {Iovino}, A. and {Lemaux}, B. and
         {L{\'o}pez-Sanjuan}, C. and {McCracken}, H.~J. and {Marano}, B. and
         {Marinoni}, C. and {Mazure}, A. and {Mellier}, Y. and {Merighi}, R. and
         {Merluzzi}, P. and {Paltani}, S. and {Pell{\`o}}, R. and {Pollo}, A. and
         {Pozzetti}, L. and {Scaramella}, R. and {Tasca}, L. and {Vergani}, D. and
         {Vettolani}, G. and {Zanichelli}, A. and {Zucca}, E.},
        title = "{The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35 016 galaxies and AGN out to z \raisebox{-0.5ex}\textasciitilde 6.7 selected with 17.5 {\ensuremath{\leq}} i$_{AB}$ {\ensuremath{\leq}} 24.75}",
      journal = {\aap},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, cosmology: observations, large-scale structure of Universe, surveys, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = nov,
       volume = {559},
          eid = {A14},
        pages = {A14},
          doi = {10.1051/0004-6361/201322179},
archivePrefix = {arXiv},
       eprint = {1307.0545},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013A&A...559A..14L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Casey12,
       author = {{Casey}, C.~M. and {Berta}, S. and {B{\'e}thermin}, M. and {Bock}, J. and
         {Bridge}, C. and {Budynkiewicz}, J. and {Burgarella}, D. and
         {Chapin}, E. and {Chapman}, S.~C. and {Clements}, D.~L. and
         {Conley}, A. and {Conselice}, C.~J. and {Cooray}, A. and {Farrah}, D. and
         {Hatziminaoglou}, E. and {Ivison}, R.~J. and {le Floc'h}, E. and
         {Lutz}, D. and {Magdis}, G. and {Magnelli}, B. and {Oliver}, S.~J. and
         {Page}, M.~J. and {Pozzi}, F. and {Rigopoulou}, D. and {Riguccini}, L. and
         {Roseboom}, I.~G. and {Sanders}, D.~B. and {Scott}, Douglas and
         {Seymour}, N. and {Valtchanov}, I. and {Vieira}, J.~D. and {Viero}, M. and
         {Wardlow}, J.},
        title = "{A Redshift Survey of Herschel Far-infrared Selected Starbursts and Implications for Obscured Star Formation}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: high-redshift, galaxies: starburst, infrared: galaxies, submillimeter: galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2012,
        month = dec,
       volume = {761},
       number = {2},
          eid = {140},
        pages = {140},
          doi = {10.1088/0004-637X/761/2/140},
archivePrefix = {arXiv},
       eprint = {1210.4928},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012ApJ...761..140C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{onodera12_passive,
       author = {{Onodera}, M. and {Renzini}, A. and {Carollo}, M. and {Cappellari}, M. and
         {Mancini}, C. and {Strazzullo}, V. and {Daddi}, E. and {Arimoto}, N. and
         {Gobat}, R. and {Yamada}, Y. and {McCracken}, H.~J. and {Ilbert}, O. and
         {Capak}, P. and {Cimatti}, A. and {Giavalisco}, M. and
         {Koekemoer}, A.~M. and {Kong}, X. and {Lilly}, S. and {Motohara}, K. and
         {Ohta}, K. and {Sanders}, D.~B. and {Scoville}, N. and {Tamura}, N. and
         {Taniguchi}, Y.},
        title = "{Deep Near-infrared Spectroscopy of Passively Evolving Galaxies at z \&gt;\raisebox{-0.5ex}\textasciitilde 1.4}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2012,
        month = aug,
       volume = {755},
       number = {1},
          eid = {26},
        pages = {26},
          doi = {10.1088/0004-637X/755/1/26},
archivePrefix = {arXiv},
       eprint = {1206.1540},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012ApJ...755...26O},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@BOOK{hoaglin83_MAD,
    author = {{Hoaglin}, D.~C. and {Mosteller}, F. and {Tukey}, J.~W.},
    title = "{Understanding robust and exploratory data analysis}",
    booktitle = {Wiley Series in Probability and Mathematical Statistics, New York: Wiley, 1983, edited by Hoaglin, David C.; Mosteller, Frederick; Tukey, John W.},
    publisher = {John Wiley,},
    series = {Wiley Series in Probability and Mathematical Statistics,},
    year = 1983,
    adsurl = {http://adsabs.harvard.edu/abs/1983ured.book.....H},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{brammer08_eazy,
       author = {{Brammer}, Gabriel B. and {van Dokkum}, Pieter G. and {Coppi}, Paolo},
        title = "{EAZY: A Fast, Public Photometric Redshift Code}",
      journal = {\apj},
     keywords = {cosmology: observations, galaxies: evolution, galaxies: formation, Astrophysics},
         year = 2008,
        month = oct,
       volume = {686},
       number = {2},
        pages = {1503-1513},
          doi = {10.1086/591786},
archivePrefix = {arXiv},
       eprint = {0807.1533},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2008ApJ...686.1503B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{quadri10_photoz_accuracy,
       author = {{Quadri}, Ryan F. and {Williams}, Rik J.},
        title = "{Quantifying Photometric Redshift Errors in the Absence of Spectroscopic Redshifts}",
      journal = {\apj},
     keywords = {cosmology: observations, galaxies: distances and redshifts, methods: miscellaneous, surveys, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2010,
        month = dec,
       volume = {725},
       number = {1},
        pages = {794-802},
          doi = {10.1088/0004-637X/725/1/794},
archivePrefix = {arXiv},
       eprint = {0910.2704},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010ApJ...725..794Q},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{laigle19_horizonAGN,
       author = {{Laigle}, C. and {Davidzon}, I. and {Ilbert}, O. and {Devriendt}, J. and
         {Kashino}, D. and {Pichon}, C. and {Capak}, P. and {Arnouts}, S. and
         {de la Torre}, S. and {Dubois}, Y. and {Gozaliasl}, G. and
         {Le Borgne}, D. and {Lilly}, S. and {McCracken}, H.~J. and
         {Salvato}, M. and {Slyz}, A.},
        title = "{Horizon-AGN virtual observatory - 1. SED-fitting performance and forecasts for future imaging surveys}",
      journal = {\mnras},
     keywords = {methods: observational, techniques: photometric, galaxies: evolution, galaxies: formation, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2019,
        month = jul,
       volume = {486},
       number = {4},
        pages = {5104-5123},
          doi = {10.1093/mnras/stz1054},
archivePrefix = {arXiv},
       eprint = {1903.10934},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.5104L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{2003SPIE.4841...72B,
       author = {{Boulade}, Olivier and {Charlot}, Xavier and {Abbon}, P. and
         {Aune}, Stephan and {Borgeaud}, Pierre and {Carton}, Pierre-Henri and
         {Carty}, M. and {Da Costa}, J. and {Deschamps}, H. and {Desforge}, D. and
         {Eppell{\'e}}, Dominique and {Gallais}, Pascal and {Gosset}, L. and
         {Granelli}, Remy and {Gros}, Michel and {de Kat}, Jean and
         {Loiseau}, Denis and {Ritou}, J. -. and {Rouss{\'e}}, Jean Y. and
         {Starzynski}, Pierre and {Vignal}, Nicolas and {Vigroux}, Laurent G.},
        title = "{MegaCam: the new Canada-France-Hawaii Telescope wide-field imaging camera}",
    booktitle = {\procspie},
         year = 2003,
       editor = {{Iye}, Masanori and {Moorwood}, Alan F.~M.},
       series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
       volume = {4841},
        month = mar,
        pages = {72-81},
          doi = {10.1117/12.459890},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2003SPIE.4841...72B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{2003SPIE.4841.1670L,
       author = {{Le F{\`e}vre}, Oliver and {Saisse}, Michel and {Mancini}, Dario and
         {Brau-Nogue}, Sylvie and {Caputi}, Oreste and {Castinel}, Louis and
         {D'Odorico}, Sandro and {Garilli}, Bianca and {Kissler-Patig}, Markus and
         {Lucuix}, Christian and {Mancini}, Guido and {Pauget}, Alain and
         {Sciarretta}, Giovanni and {Scodeggio}, Marco and {Tresse}, Laurence and
         {Vettolani}, Gianpaolo},
        title = "{Commissioning and performances of the VLT-VIMOS instrument}",
    booktitle = {\procspie},
         year = 2003,
       editor = {{Iye}, Masanori and {Moorwood}, Alan F.~M.},
       series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
       volume = {4841},
        month = mar,
        pages = {1670-1681},
          doi = {10.1117/12.460959},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2003SPIE.4841.1670L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2007Natur.445..286M,
       author = {{Massey}, Richard and {Rhodes}, Jason and {Ellis}, Richard and
         {Scoville}, Nick and {Leauthaud}, Alexie and {Finoguenov}, Alexis and
         {Capak}, Peter and {Bacon}, David and {Aussel}, Herv{\'e} and
         {Kneib}, Jean-Paul and {Koekemoer}, Anton and {McCracken}, Henry and
         {Mobasher}, Bahram and {Pires}, Sandrine and {Refregier}, Alexandre and
         {Sasaki}, Shunji and {Starck}, Jean-Luc and {Taniguchi}, Yoshi and
         {Taylor}, Andy and {Taylor}, James},
        title = "{Dark matter maps reveal cosmic scaffolding}",
      journal = {\nat},
     keywords = {Astrophysics},
         year = 2007,
        month = jan,
       volume = {445},
       number = {7125},
        pages = {286-290},
          doi = {10.1038/nature05497},
archivePrefix = {arXiv},
       eprint = {astro-ph/0701594},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007Natur.445..286M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{stockmann20_QGz2,
       author = {{Stockmann}, Mikkel and {Toft}, Sune and {Gallazzi}, Anna and
         {Zibetti}, Stefano and {Conselice}, Christopher J. and
         {Margalef-Bentabol}, Berta and {Zabl}, Johannes and
         {J{\o}rgensen}, Inger and {Magdis}, Georgios E. and
         {G{\'o}mez-Guijarro}, Carlos and {Valentino}, Francesco M. and
         {Brammer}, Gabriel B. and {Ceverino}, Daniel and {Cortzen}, Isabella and
         {Davidzon}, Iary and {Demarco}, Richardo and {Faisst}, Andreas and
         {Hirschmann}, Michaela and {Krogager}, Jens-Kristian and
         {Lagos}, Claudia D. and {Man}, Allison W.~S. and {Mundy}, Carl J. and
         {Peng}, Yingjie and {Selsing}, Jonatan and {Steinhardt}, Charles L. and
         {Whitaker}, Kathrine E.},
        title = "{X-shooter Spectroscopy and HST Imaging of 15 Massive Quiescent Galaxies at z {\ensuremath{\gtrsim}} 2}",
      journal = {\apj},
     keywords = {Infrared galaxies, Compact galaxies, Quenched galaxies, Near infrared astronomy, Infrared astronomy, Galaxy kinematics, Galaxy dynamics, Stellar masses, Stellar ages, Stellar radii, High resolution spectroscopy, Hubble Space Telescope, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = jan,
       volume = {888},
       number = {1},
          eid = {4},
        pages = {4},
          doi = {10.3847/1538-4357/ab5af4},
archivePrefix = {arXiv},
       eprint = {1912.01619},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...888....4S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Valentino20_QGz4,
       author = {{Valentino}, Francesco and {Tanaka}, Masayuki and {Davidzon}, Iary and
         {Toft}, Sune and {G{\'o}mez-Guijarro}, Carlos and {Stockmann}, Mikkel and
         {Onodera}, Masato and {Brammer}, Gabriel and {Ceverino}, Daniel and
         {Faisst}, Andreas L. and {Gallazzi}, Anna and
         {Hayward}, Christopher C. and {Ilbert}, Olivier and {Kubo}, Mariko and
         {Magdis}, Georgios E. and {Selsing}, Jonatan and {Shimakawa}, Rhythm and
         {Sparre}, Martin and {Steinhardt}, Charles and {Yabe}, Kiyoto and
         {Zabl}, Johannes},
        title = "{Quiescent Galaxies 1.5 Billion Years after the Big Bang and Their Progenitors}",
      journal = {\apj},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = feb,
       volume = {889},
       number = {2},
          eid = {93},
        pages = {93},
          doi = {10.3847/1538-4357/ab64dc},
archivePrefix = {arXiv},
       eprint = {1909.10540},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...889...93V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Schreiber18_QGz4,
       author = {{Schreiber}, C. and {Glazebrook}, K. and {Nanayakkara}, T. and
         {Kacprzak}, G.~G. and {Labb{\'e}}, I. and {Oesch}, P. and {Yuan}, T. and
         {Tran}, K. -V. and {Papovich}, C. and {Spitler}, L. and {Straatman}, C.},
        title = "{Near infrared spectroscopy and star-formation histories of 3 {\ensuremath{\leq}} z {\ensuremath{\leq}} 4 quiescent galaxies}",
      journal = {\aap},
     keywords = {techniques: spectroscopic, galaxies: evolution, galaxies: high-redshift, galaxies: statistics, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = oct,
       volume = {618},
          eid = {A85},
        pages = {A85},
          doi = {10.1051/0004-6361/201833070},
archivePrefix = {arXiv},
       eprint = {1807.02523},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018A&A...618A..85S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{leslie20_ssfr,
       author = {{Leslie}, Sarah and {Schinnerer}, Eva and {Liu}, Daizhong and
         {Magnelli}, Benjamin and {Algera}, Hiddo and {Karim}, Alexander and
         {Davidzon}, Iary and {Gozaliasl}, Ghassem and
         {Jim{\'e}nez-Andrade}, Eric F. and {Lang}, Philipp and {Sargent}, Mark and
         {Novak}, Mladen and {Groves}, Brent and {Smol{\v{c}}i{\'c}}, Vernesa and
         {Zamorani}, Giovanni and {Vaccari}, Mattia and {Battisti}, Andrew and
         {Vardoulaki}, Eleni and {Peng}, Yingjie and {Kartaltepe}, Jeyhan},
        title = "{The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to $z\sim5$}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = jun,
          eid = {arXiv:2006.13937},
        pages = {arXiv:2006.13937},
archivePrefix = {arXiv},
       eprint = {2006.13937},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020arXiv200613937L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{hasinger18_deimos10k,
       author = {{Hasinger}, G. and {Capak}, P. and {Salvato}, M. and {Barger}, A.~J. and
         {Cowie}, L.~L. and {Faisst}, A. and {Hemmati}, S. and {Kakazu}, Y. and
         {Kartaltepe}, J. and {Masters}, D. and {Mobasher}, B. and
         {Nayyeri}, H. and {Sanders}, D. and {Scoville}, N.~Z. and {Suh}, H. and
         {Steinhardt}, C. and {Yang}, Fengwei},
        title = "{The DEIMOS 10K Spectroscopic Survey Catalog of the COSMOS Field}",
      journal = {\apj},
     keywords = {catalogs, galaxies: distances and redshifts, surveys, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2018,
        month = may,
       volume = {858},
       number = {2},
          eid = {77},
        pages = {77},
          doi = {10.3847/1538-4357/aabacf},
archivePrefix = {arXiv},
       eprint = {1803.09251},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ApJ...858...77H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@article{Hsieh_2012,
	doi = {10.1088/0067-0049/203/2/23},
	url = {https://doi.org/10.1088%2F0067-0049%2F203%2F2%2F23},
	year = 2012,
	month = {nov},
	publisher = {{IOP} Publishing},
	volume = {203},
	number = {2},
	pages = {23},
	author = {Bau-Ching Hsieh and Wei-Hao Wang and Chih-Chiang Hsieh and Lihwai Lin and Haojing Yan and Jeremy Lim and Paul T. P. Ho},
	title = {{THE} {TAIWAN} {ECDFS} {NEAR}-{INFRARED} {SURVEY}: {ULTRA}-{DEEP}
		                    J
		                    {AND}
		                    
		                      K
		                      S
		                    
		                    {IMAGING} {IN} {THE} {EXTENDED} {CHANDRA} {DEEP} {FIELD}-{SOUTH}},
	journal = {The Astrophysical Journal Supplement Series},
	abstract = {We present ultra-deep J and KS
             imaging observations covering a 30′ × 30′ area of the Extended Chandra Deep Field-South (ECDFS) carried out by our Taiwan ECDFS Near-Infrared Survey (TENIS). The median 5σ limiting magnitudes for all detected objects in the ECDFS reach 24.5 and 23.9 mag (AB) for J and KS
            , respectively. In the inner 400 arcmin2 region where the sensitivity is more uniform, objects as faint as 25.6 and 25.0 mag are detected at 5σ. Thus, this is by far the deepest J and KS
             data sets available for the ECDFS. To combine TENIS with the Spitzer IRAC data for obtaining better spectral energy distributions of high-redshift objects, we developed a novel deconvolution technique (IRACLEAN) to accurately estimate the IRAC fluxes. IRACLEAN can minimize the effect of blending in the IRAC images caused by the large point-spread functions and reduce the confusion noise. We applied IRACLEAN to the images from the Spitzer IRAC/MUSYC Public Legacy in the ECDFS survey (SIMPLE) and generated a J+KS
            -selected multi-wavelength catalog including the photometry of both the TENIS near-infrared and the SIMPLE IRAC data. We publicly release the data products derived from this work, including the J and KS
             images and the J+KS
            -selected multi-wavelength catalog.}
}


@ARTICLE{Coupon_HSC_Masks_2018,
       author = {{Coupon}, Jean and {Czakon}, Nicole and {Bosch}, James and
         {Komiyama}, Yutaka and {Medezinski}, Elinor and {Miyazaki}, Satoshi and
         {Oguri}, Masamune},
        title = "{The bright-star masks for the HSC-SSP survey}",
      journal = {\pasj},
     keywords = {cosmology: observations, galaxies: photometry, techniques: image processing, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2018,
        month = jan,
       volume = {70},
          eid = {S7},
        pages = {S7},
     abstract = "{We present the procedure to build and validate the bright-star masks for
        the Hyper-Suprime-Cam Strategic Subaru Proposal (HSC-SSP)
        survey. To identify and mask the saturated stars in the full
        HSC-SSP footprint, we rely on the Gaia and Tycho-2 star
        catalogues. We first assemble a pure star catalogue down to
        G$_{Gaia}$ $\lt$ 18 after removing {\ensuremath{\sim}}1.5\% of
        sources that appear extended in the Sloan Digital Sky Survey
        (SDSS). We perform visual inspection on the early data from the
        S16A internal release of HSC-SSP, finding that our star
        catalogue is 99.2\% pure down to G$_{Gaia}$ $\lt$ 18. Second, we
        build the mask regions in an automated way using stacked
        detected source measurements around bright stars binned per
        G$_{Gaia}$ magnitude. Finally, we validate those masks by visual
        inspection and comparison with the literature of galaxy number
        counts and angular two-point correlation functions. This version
        (Arcturus) supersedes the previous version (Sirius) used in the
        S16A internal and DR1 public releases. We publicly release the
        full masks and tools to flag objects in the entire footprint of
        the planned HSC-SSP observations at
        ``ftp://obsftp.unige.ch/pub/coupon/brightStarMasks/HSC-SSP/''.}",
          doi = {10.1093/pasj/psx047},
archivePrefix = {arXiv},
       eprint = {1705.00622},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018PASJ...70S...7C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{1999AJ....117...68S,
       author = {{Szalay}, Alexander S. and {Connolly}, Andrew J. and {Szokoly}, Gyula P.},
        title = "{Simultaneous Multicolor Detection of Faint Galaxies in the Hubble Deep Field}",
      journal = {\aj},
     keywords = {COSMOLOGY: OBSERVATIONS, GALAXIES: FUNDAMENTAL PARAMETERS, GALAXIES: PHOTOMETRY, TECHNIQUES: PHOTOMETRIC, Astrophysics},
         year = 1999,
        month = jan,
       volume = {117},
       number = {1},
        pages = {68-74},
          doi = {10.1086/300689},
archivePrefix = {arXiv},
       eprint = {astro-ph/9811086},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1999AJ....117...68S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2014PASP..126..158G,
       author = {{Gruen}, D. and {Seitz}, S. and {Bernstein}, G.~M.},
        title = "{Implementation of Robust Image Artifact Removal in SWarp through Clipped Mean Stacking}",
      journal = {\pasp},
     keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2014,
        month = feb,
       volume = {126},
       number = {936},
        pages = {158},
          doi = {10.1086/675080},
archivePrefix = {arXiv},
       eprint = {1401.4169},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014PASP..126..158G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{1888BuAsI...5..303B,
       author = {{Bigourdan}, G.},
        title = "{Revue des publications astronomiques. Bulletin du comit{\'e} international permanent pour l'ex{\'e}cution photographique de la Carte du Ciel. Premier fascicule}",
      journal = {Bulletin Astronomique, Serie I},
         year = 1888,
        month = jan,
       volume = {5},
        pages = {303-309},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1888BuAsI...5..303B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{1934ApJ....79....8H,
       author = {{Hubble}, Edwin},
        title = "{The Distribution of Extra-Galactic Nebulae}",
      journal = {\apj},
         year = 1934,
        month = jan,
       volume = {79},
        pages = {8},
          doi = {10.1086/143517},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1934ApJ....79....8H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{1988AJ.....96....1T,
       author = {{Tyson}, J.~A.},
        title = "{Deep CCD Survey: Galaxy Luminosity and Color Evolution}",
      journal = {\aj},
     keywords = {Charge Coupled Devices, Color-Magnitude Diagram, Galactic Evolution, Red Shift, Sky Surveys (Astronomy), Ultraviolet Radiation, Dark Matter, Perturbation Theory, Stellar Evolution, Stellar Mass, Astrophysics, GALAXIES: GENERAL, COSMOLOGY},
         year = 1988,
        month = jul,
       volume = {96},
        pages = {1},
          doi = {10.1086/114786},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1988AJ.....96....1T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2004PASP..116..449M,
       author = {{Magnier}, E.~A. and {Cuillandre}, J. -C.},
        title = "{The Elixir System: Data Characterization and Calibration at the Canada-France-Hawaii Telescope}",
      journal = {\pasp},
     keywords = {Techniques: Image Processing, astronomical databases: miscellaneous},
         year = 2004,
        month = may,
       volume = {116},
       number = {819},
        pages = {449-464},
          doi = {10.1086/420756},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2004PASP..116..449M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2011ApJS..193...29A,
       author = {{Aihara}, Hiroaki and {Allende Prieto}, Carlos and {An}, Deokkeun and
         {Anderson}, Scott F. and {Aubourg}, {\'E}ric and {Balbinot}, Eduardo and
         {Beers}, Timothy C. and {Berlind}, Andreas A. and
         {Bickerton}, Steven J. and {Bizyaev}, Dmitry and {Blanton}, Michael R. and
         {Bochanski}, John J. and {Bolton}, Adam S. and {Bovy}, Jo and {Brand
        t}, W.~N. and {Brinkmann}, J. and {Brown}, Peter J. and
         {Brownstein}, Joel R. and {Busca}, Nicolas G. and {Campbell}, Heather and
         {Carr}, Michael A. and {Chen}, Yanmei and {Chiappini}, Cristina and
         {Comparat}, Johan and {Connolly}, Natalia and {Cortes}, Marina and
         {Croft}, Rupert A.~C. and {Cuesta}, Antonio J. and {da Costa}, Luiz N. and
         {Davenport}, James R.~A. and {Dawson}, Kyle and {Dhital}, Saurav and
         {Ealet}, Anne and {Ebelke}, Garrett L. and {Edmondson}, Edward M. and
         {Eisenstein}, Daniel J. and {Escoffier}, Stephanie and
         {Esposito}, Massimiliano and {Evans}, Michael L. and {Fan}, Xiaohui and
         {Femen{\'\i}a Castell{\'a}}, Bruno and {Font-Ribera}, Andreu and
         {Frinchaboy}, Peter M. and {Ge}, Jian and {Gillespie}, Bruce A. and
         {Gilmore}, G. and {Gonz{\'a}lez Hern{\'a}ndez}, Jonay I. and
         {Gott}, J. Richard and {Gould}, Andrew and {Grebel}, Eva K. and
         {Gunn}, James E. and {Hamilton}, Jean-Christophe and {Harding}, Paul and
         {Harris}, David W. and {Hawley}, Suzanne L. and {Hearty}, Frederick R. and
         {Ho}, Shirley and {Hogg}, David W. and {Holtzman}, Jon A. and
         {Honscheid}, Klaus and {Inada}, Naohisa and {Ivans}, Inese I. and
         {Jiang}, Linhua and {Johnson}, Jennifer A. and {Jordan}, Cathy and
         {Jordan}, Wendell P. and {Kazin}, Eyal A. and {Kirkby}, David and
         {Klaene}, Mark A. and {Knapp}, G.~R. and {Kneib}, Jean-Paul and
         {Kochanek}, C.~S. and {Koesterke}, Lars and {Kollmeier}, Juna A. and
         {Kron}, Richard G. and {Lampeitl}, Hubert and {Lang}, Dustin and
         {Le Goff}, Jean-Marc and {Lee}, Young Sun and {Lin}, Yen-Ting and
         {Long}, Daniel C. and {Loomis}, Craig P. and {Lucatello}, Sara and
         {Lundgren}, Britt and {Lupton}, Robert H. and {Ma}, Zhibo and
         {MacDonald}, Nicholas and {Mahadevan}, Suvrath and
         {Maia}, Marcio A.~G. and {Makler}, Martin and {Malanushenko}, Elena and
         {Malanushenko}, Viktor and {Mandelbaum}, Rachel and
         {Maraston}, Claudia and {Margala}, Daniel and {Masters}, Karen L. and
         {McBride}, Cameron K. and {McGehee}, Peregrine M. and
         {McGreer}, Ian D. and {M{\'e}nard}, Brice and
         {Miralda-Escud{\'e}}, Jordi and {Morrison}, Heather L. and
         {Mullally}, F. and {Muna}, Demitri and {Munn}, Jeffrey A. and
         {Murayama}, Hitoshi and {Myers}, Adam D. and {Naugle}, Tracy and
         {Neto}, Angelo Fausti and {Nguyen}, Duy Cuong and {Nichol}, Robert C. and
         {O'Connell}, Robert W. and {Ogando}, Ricardo L.~C. and
         {Olmstead}, Matthew D. and {Oravetz}, Daniel J. and
         {Padmanabhan}, Nikhil and {Palanque-Delabrouille}, Nathalie and
         {Pan}, Kaike and {Pandey}, Parul and {P{\^a}ris}, Isabelle and
         {Percival}, Will J. and {Petitjean}, Patrick and
         {Pfaffenberger}, Robert and {Pforr}, Janine and {Phleps}, Stefanie and
         {Pichon}, Christophe and {Pieri}, Matthew M. and {Prada}, Francisco and
         {Price-Whelan}, Adrian M. and {Raddick}, M. Jordan and
         {Ramos}, Beatriz H.~F. and {Reyl{\'e}}, C{\'e}line and {Rich}, James and
         {Richards}, Gordon T. and {Rix}, Hans-Walter and {Robin}, Annie C. and
         {Rocha-Pinto}, Helio J. and {Rockosi}, Constance M. and
         {Roe}, Natalie A. and {Rollinde}, Emmanuel and {Ross}, Ashley J. and
         {Ross}, Nicholas P. and {Rossetto}, Bruno M. and
         {S{\'a}nchez}, Ariel G. and {Sayres}, Conor and {Schlegel}, David J. and
         {Schlesinger}, Katharine J. and {Schmidt}, Sarah J. and
         {Schneider}, Donald P. and {Sheldon}, Erin and {Shu}, Yiping and
         {Simmerer}, Jennifer and {Simmons}, Audrey E. and
         {Sivarani}, Thirupathi and {Snedden}, Stephanie A. and
         {Sobeck}, Jennifer S. and {Steinmetz}, Matthias and
         {Strauss}, Michael A. and {Szalay}, Alexander S. and
         {Tanaka}, Masayuki and {Thakar}, Aniruddha R. and {Thomas}, Daniel and
         {Tinker}, Jeremy L. and {Tofflemire}, Benjamin M. and {Tojeiro}, Rita and
         {Tremonti}, Christy A. and {Vandenberg}, Jan and
         {Vargas Maga{\~n}a}, M. and {Verde}, Licia and {Vogt}, Nicole P. and
         {Wake}, David A. and {Wang}, Ji and {Weaver}, Benjamin A. and
         {Weinberg}, David H. and {White}, Martin and {White}, Simon D.~M. and
         {Yanny}, Brian and {Yasuda}, Naoki and {Yeche}, Christophe and
         {Zehavi}, Idit},
        title = "{The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III}",
      journal = {\apjs},
     keywords = {atlases, catalogs, surveys, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2011,
        month = apr,
       volume = {193},
       number = {2},
          eid = {29},
        pages = {29},
          doi = {10.1088/0067-0049/193/2/29},
archivePrefix = {arXiv},
       eprint = {1101.1559},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJS..193...29A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2012A&A...545A..23B,
       author = {{Bielby}, R. and {Hudelot}, P. and {McCracken}, H.~J. and {Ilbert}, O. and
         {Daddi}, E. and {Le F{\`e}vre}, O. and {Gonzalez-Perez}, V. and
         {Kneib}, J. -P. and {Marmo}, C. and {Mellier}, Y. and {Salvato}, M. and
         {Sanders}, D.~B. and {Willott}, C.~J.},
        title = "{The WIRCam Deep Survey. I. Counts, colours, and mass-functions derived from near-infrared imaging in the CFHTLS deep fields}",
      journal = {\aap},
     keywords = {catalogs, surveys, cosmology: observations, galaxies: evolution, galaxies: luminosity function, mass function, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2012,
        month = sep,
       volume = {545},
          eid = {A23},
        pages = {A23},
          doi = {10.1051/0004-6361/201118547},
archivePrefix = {arXiv},
       eprint = {1111.6997},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012A&A...545A..23B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2014A&A...570A..11F,
       author = {{Fontana}, A. and {Dunlop}, J.~S. and {Paris}, D. and {Targett}, T.~A. and
         {Boutsia}, K. and {Castellano}, M. and {Galametz}, A. and
         {Grazian}, A. and {McLure}, R. and {Merlin}, E. and {Pentericci}, L. and
         {Wuyts}, S. and {Almaini}, O. and {Caputi}, K. and {Chary}, R. -R. and
         {Cirasuolo}, M. and {Conselice}, C.~J. and {Cooray}, A. and
         {Daddi}, E. and {Dickinson}, M. and {Faber}, S.~M. and {Fazio}, G. and
         {Ferguson}, H.~C. and {Giallongo}, E. and {Giavalisco}, M. and
         {Grogin}, N.~A. and {Hathi}, N. and {Koekemoer}, A.~M. and
         {Koo}, D.~C. and {Lucas}, R.~A. and {Nonino}, M. and {Rix}, H.~W. and
         {Renzini}, A. and {Rosario}, D. and {Santini}, P. and {Scarlata}, C. and
         {Sommariva}, V. and {Stark}, D.~P. and {van der Wel}, A. and
         {Vanzella}, E. and {Wild}, V. and {Yan}, H. and {Zibetti}, S.},
        title = "{The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts}",
      journal = {\aap},
     keywords = {surveys, galaxies: evolution, Astrophysics - Astrophysics of Galaxies},
         year = 2014,
        month = oct,
       volume = {570},
          eid = {A11},
        pages = {A11},
          doi = {10.1051/0004-6361/201423543},
archivePrefix = {arXiv},
       eprint = {1409.7082},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014A&A...570A..11F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2015A&A...582A..15M,
       author = {{Merlin}, E. and {Fontana}, A. and {Ferguson}, H.~C. and
         {Dunlop}, J.~S. and {Elbaz}, D. and {Bourne}, N. and {Bruce}, V.~A. and
         {Buitrago}, F. and {Castellano}, M. and {Schreiber}, C. and
         {Grazian}, A. and {McLure}, R.~J. and {Okumura}, K. and {Shu}, X. and
         {Wang}, T. and {Amor{\'\i}n}, R. and {Boutsia}, K. and
         {Cappelluti}, N. and {Comastri}, A. and {Derriere}, S. and
         {Faber}, S.~M. and {Santini}, P.},
        title = "{T-PHOT: A new code for PSF-matched, prior-based, multiwavelength extragalactic deconfusion photometry}",
      journal = {\aap},
     keywords = {techniques: photometric, galaxies: photometry, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2015,
        month = oct,
       volume = {582},
          eid = {A15},
        pages = {A15},
          doi = {10.1051/0004-6361/201526471},
archivePrefix = {arXiv},
       eprint = {1505.02516},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015A&A...582A..15M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2016A&A...595A..97M,
       author = {{Merlin}, E. and {Bourne}, N. and {Castellano}, M. and
         {Ferguson}, H.~C. and {Wang}, T. and {Derriere}, S. and
         {Dunlop}, J.~S. and {Elbaz}, D. and {Fontana}, A.},
        title = "{T-PHOT version 2.0: Improved algorithms for background subtraction, local convolution, kernel registration, and new options}",
      journal = {\aap},
     keywords = {methods: data analysis, techniques: photometric, galaxies: photometry, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = nov,
       volume = {595},
          eid = {A97},
        pages = {A97},
          doi = {10.1051/0004-6361/201628751},
archivePrefix = {arXiv},
       eprint = {1609.00146},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016A&A...595A..97M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2013PASP..125.1514M,
       author = {{Mancone}, Conor L. and {Gonzalez}, Anthony H. and
         {Moustakas}, Leonidas A. and {Price}, Andrew},
        title = "{PyGFit: A Tool for Extracting PSF Matched Photometry}",
      journal = {\pasp},
     keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = dec,
       volume = {125},
       number = {934},
        pages = {1514},
          doi = {10.1086/674431},
archivePrefix = {arXiv},
       eprint = {1310.6046},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013PASP..125.1514M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2016MNRAS.460..765W,
       author = {{Wright}, A.~H. and {Robotham}, A.~S.~G. and {Bourne}, N. and
         {Driver}, S.~P. and {Dunne}, L. and {Maddox}, S.~J. and {Alpaslan}, M. and
         {Andrews}, S.~K. and {Bauer}, A.~E. and {Bland-Hawthorn}, J. and
         {Brough}, S. and {Brown}, M.~J.~I. and {Clarke}, C. and {Cluver}, M. and
         {Davies}, L.~J.~M. and {Grootes}, M.~W. and {Holwerda}, B.~W. and
         {Hopkins}, A.~M. and {Jarrett}, T.~H. and {Kafle}, P.~R. and
         {Lange}, R. and {Liske}, J. and {Loveday}, J. and {Moffett}, A.~J. and
         {Norberg}, P. and {Popescu}, C.~C. and {Smith}, M. and {Taylor}, E.~N. and
         {Tuffs}, R.~J. and {Wang}, L. and {Wilkins}, S.~M.},
        title = "{Galaxy And Mass Assembly: accurate panchromatic photometry from optical priors using LAMBDAR}",
      journal = {\mnras},
     keywords = {techniques: photometric, astronomical data bases: miscellaneous, galaxies: evolution, galaxies: general, galaxies: photometry, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = jul,
       volume = {460},
       number = {1},
        pages = {765-801},
          doi = {10.1093/mnras/stw832},
archivePrefix = {arXiv},
       eprint = {1604.01923},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016MNRAS.460..765W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2016AJ....151...36L,
       author = {{Lang}, Dustin and {Hogg}, David W. and {Schlegel}, David J.},
        title = "{WISE Photometry for 400 Million SDSS Sources}",
      journal = {\aj},
     keywords = {catalogs, methods: data analysis, surveys, techniques: image processing},
         year = 2016,
        month = feb,
       volume = {151},
       number = {2},
          eid = {36},
        pages = {36},
          doi = {10.3847/0004-6256/151/2/36},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016AJ....151...36L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{1998PASP..110..863P,
       author = {{Pickles}, A.~J.},
        title = "{A Stellar Spectral Flux Library: 1150-25000 {\r{A}}}",
      journal = {\pasp},
     keywords = {ATLASES, STARS: GENERAL, GALAXIES: STELLAR CONTENT},
         year = 1998,
        month = jul,
       volume = {110},
       number = {749},
        pages = {863-878},
          doi = {10.1086/316197},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1998PASP..110..863P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{1995AJ....110.1316B,
       author = {{Bohlin}, Ralph C. and {Colina}, Luis and {Finley}, David S.},
        title = "{White Dwarf Standard Stars: G191-B2B, GD 71, GD 153, HZ 43}",
      journal = {\aj},
     keywords = {WHITE DWARFS, STARS: FUNDAMENTAL PARAMETERS},
         year = 1995,
        month = sep,
       volume = {110},
        pages = {1316},
          doi = {10.1086/117606},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1995AJ....110.1316B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2015A&A...577A..42B,
       author = {{Baraffe}, Isabelle and {Homeier}, Derek and {Allard}, France and
         {Chabrier}, Gilles},
        title = "{New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit}",
      journal = {\aap},
     keywords = {stars: evolution, stars: low-mass, stars: pre-main sequence, Hertzsprung-Russell and C-M diagrams, convection, Astrophysics - Solar and Stellar Astrophysics},
         year = 2015,
        month = may,
       volume = {577},
          eid = {A42},
        pages = {A42},
          doi = {10.1051/0004-6361/201425481},
archivePrefix = {arXiv},
       eprint = {1503.04107},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015A&A...577A..42B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2000ApJ...542..464C,
       author = {{Chabrier}, G. and {Baraffe}, I. and {Allard}, F. and {Hauschildt}, P.},
        title = "{Evolutionary Models for Very Low-Mass Stars and Brown Dwarfs with Dusty Atmospheres}",
      journal = {\apj},
     keywords = {Hertzsprung-Russell, Stars: Evolution, Stars: Low-Mass, Brown Dwarfs, Stars: Luminosity Function, Mass Function, Astrophysics},
         year = 2000,
        month = oct,
       volume = {542},
       number = {1},
        pages = {464-472},
          doi = {10.1086/309513},
archivePrefix = {arXiv},
       eprint = {astro-ph/0005557},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2000ApJ...542..464C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2012ApJ...756..172M,
       author = {{Morley}, Caroline V. and {Fortney}, Jonathan J. and {Marley}, Mark S. and
         {Visscher}, Channon and {Saumon}, Didier and {Leggett}, S.~K.},
        title = "{Neglected Clouds in T and Y Dwarf Atmospheres}",
      journal = {\apj},
     keywords = {brown dwarfs, stars: atmospheres, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics},
         year = 2012,
        month = sep,
       volume = {756},
       number = {2},
          eid = {172},
        pages = {172},
          doi = {10.1088/0004-637X/756/2/172},
archivePrefix = {arXiv},
       eprint = {1206.4313},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012ApJ...756..172M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2014ApJ...787...78M,
       author = {{Morley}, Caroline V. and {Marley}, Mark S. and {Fortney}, Jonathan J. and
         {Lupu}, Roxana and {Saumon}, Didier and {Greene}, Tom and
         {Lodders}, Katharina},
        title = "{Water Clouds in Y Dwarfs and Exoplanets}",
      journal = {\apj},
     keywords = {brown dwarfs, planets and satellites: atmospheres, planets and satellites: detection, stars: atmospheres, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics},
         year = 2014,
        month = may,
       volume = {787},
       number = {1},
          eid = {78},
        pages = {78},
          doi = {10.1088/0004-637X/787/1/78},
archivePrefix = {arXiv},
       eprint = {1404.0005},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014ApJ...787...78M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2008ApJ...689.1327S,
       author = {{Saumon}, D. and {Marley}, Mark S.},
        title = "{The Evolution of L and T Dwarfs in Color-Magnitude Diagrams}",
      journal = {\apj},
     keywords = {stars: atmospheres, stars: evolution, stars: low-mass, brown dwarfs, Astrophysics},
         year = 2008,
        month = dec,
       volume = {689},
       number = {2},
        pages = {1327-1344},
          doi = {10.1086/592734},
archivePrefix = {arXiv},
       eprint = {0808.2611},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2008ApJ...689.1327S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2018PASJ...70S...1M,
       author = {{Miyazaki}, Satoshi and {Komiyama}, Yutaka and {Kawanomoto}, Satoshi and
         {Doi}, Yoshiyuki and {Furusawa}, Hisanori and {Hamana}, Takashi and
         {Hayashi}, Yusuke and {Ikeda}, Hiroyuki and {Kamata}, Yukiko and
         {Karoji}, Hiroshi and {Koike}, Michitaro and {Kurakami}, Tomio and
         {Miyama}, Shoken and {Morokuma}, Tomoki and {Nakata}, Fumiaki and
         {Namikawa}, Kazuhito and {Nakaya}, Hidehiko and {Nariai}, Kyoji and
         {Obuchi}, Yoshiyuki and {Oishi}, Yukie and {Okada}, Norio and
         {Okura}, Yuki and {Tait}, Philip and {Takata}, Tadafumi and
         {Tanaka}, Yoko and {Tanaka}, Masayuki and {Terai}, Tsuyoshi and
         {Tomono}, Daigo and {Uraguchi}, Fumihiro and {Usuda}, Tomonori and
         {Utsumi}, Yousuke and {Yamada}, Yoshihiko and {Yamanoi}, Hitomi and
         {Aihara}, Hiroaki and {Fujimori}, Hiroki and {Mineo}, Sogo and
         {Miyatake}, Hironao and {Oguri}, Masamune and {Uchida}, Tomohisa and
         {Tanaka}, Manobu M. and {Yasuda}, Naoki and {Takada}, Masahiro and
         {Murayama}, Hitoshi and {Nishizawa}, Atsushi J. and {Sugiyama}, Naoshi and
         {Chiba}, Masashi and {Futamase}, Toshifumi and {Wang}, Shiang-Yu and
         {Chen}, Hsin-Yo and {Ho}, Paul T.~P. and {Liaw}, Eric J.~Y. and
         {Chiu}, Chi-Fang and {Ho}, Cheng-Lin and {Lai}, Tsang-Chih and
         {Lee}, Yao-Cheng and {Jeng}, Dun-Zen and {Iwamura}, Satoru and
         {Armstrong}, Robert and {Bickerton}, Steve and {Bosch}, James and
         {Gunn}, James E. and {Lupton}, Robert H. and {Loomis}, Craig and
         {Price}, Paul and {Smith}, Steward and {Strauss}, Michael A. and
         {Turner}, Edwin L. and {Suzuki}, Hisanori and {Miyazaki}, Yasuhito and
         {Muramatsu}, Masaharu and {Yamamoto}, Koei and {Endo}, Makoto and
         {Ezaki}, Yutaka and {Ito}, Noboru and {Kawaguchi}, Noboru and
         {Sofuku}, Satoshi and {Taniike}, Tomoaki and {Akutsu}, Kotaro and
         {Dojo}, Naoto and {Kasumi}, Kazuyuki and {Matsuda}, Toru and
         {Imoto}, Kohei and {Miwa}, Yoshinori and {Suzuki}, Masayuki and
         {Takeshi}, Kunio and {Yokota}, Hideo},
        title = "{Hyper Suprime-Cam: System design and verification of image quality}",
      journal = {\pasj},
     keywords = {instrumentation: detectors, techniques: image processing, telescopes},
         year = 2018,
        month = jan,
       volume = {70},
          eid = {S1},
        pages = {S1},
          doi = {10.1093/pasj/psx063},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018PASJ...70S...1M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@INPROCEEDINGS{2006ASPC..351..112B,
       author = {{Bertin}, E.},
        title = "{Automatic Astrometric and Photometric Calibration with SCAMP}",
    booktitle = {Astronomical Data Analysis Software and Systems XV},
         year = 2006,
       editor = {{Gabriel}, C. and {Arviset}, C. and {Ponz}, D. and {Enrique}, S.},
       series = {Astronomical Society of the Pacific Conference Series},
       volume = {351},
        month = jul,
        pages = {112},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2006ASPC..351..112B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2020AJ....159..165P,
       author = {{Portillo}, Stephen K.~N. and {Speagle}, Joshua S. and
         {Finkbeiner}, Douglas P.},
        title = "{Photometric Biases in Modern Surveys}",
      journal = {\aj},
     keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2020,
        month = apr,
       volume = {159},
       number = {4},
          eid = {165},
        pages = {165},
          doi = {10.3847/1538-3881/ab76ba},
archivePrefix = {arXiv},
       eprint = {1902.02374},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020AJ....159..165P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{milvangjensen_2013,
       author = {{Milvang-Jensen}, Bo and {Freudling}, Wolfram and {Zabl}, Johannes and
         {Fynbo}, Johan P.~U. and {M{\o}ller}, Palle and {Nilsson}, Kim K. and
         {McCracken}, Henry Joy and {Hjorth}, Jens and {Le F{\`e}vre}, Olivier and
         {Tasca}, Lidia and {Dunlop}, James S. and {Sobral}, David},
        title = "{On-sky characterisation of the VISTA NB118 narrow-band filters at 1.19 {\ensuremath{\mu}}m}",
      journal = {\aap},
     keywords = {techniques: photometric, instrumentation: photometers, methods: observational, galaxies: photometry, galaxies: high-redshift, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - Galaxy Astrophysics},
         year = 2013,
        month = dec,
       volume = {560},
          eid = {A94},
        pages = {A94},
          doi = {10.1051/0004-6361/201321814},
archivePrefix = {arXiv},
       eprint = {1305.0262},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013A&A...560A..94M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{dey2019_decals,
       author = {{Dey}, Arjun and {Schlegel}, David J. and {Lang}, Dustin and
         {Blum}, Robert and {Burleigh}, Kaylan and {Fan}, Xiaohui and
         {Findlay}, Joseph R. and {Finkbeiner}, Doug and {Herrera}, David and
         {Juneau}, St{\'e}phanie and {Landriau}, Martin and {Levi}, Michael and
         {McGreer}, Ian and {Meisner}, Aaron and {Myers}, Adam D. and
         {Moustakas}, John and {Nugent}, Peter and {Patej}, Anna and
         {Schlafly}, Edward F. and {Walker}, Alistair R. and
         {Valdes}, Francisco and {Weaver}, Benjamin A. and
         {Y{\`e}che}, Christophe and {Zou}, Hu and {Zhou}, Xu and
         {Abareshi}, Behzad and {Abbott}, T.~M.~C. and {Abolfathi}, Bela and
         {Aguilera}, C. and {Alam}, Shadab and {Allen}, Lori and {Alvarez}, A. and
         {Annis}, James and {Ansarinejad}, Behzad and {Aubert}, Marie and
         {Beechert}, Jacqueline and {Bell}, Eric F. and {BenZvi}, Segev Y. and
         {Beutler}, Florian and {Bielby}, Richard M. and {Bolton}, Adam S. and
         {Brice{\~n}o}, C{\'e}sar and {Buckley-Geer}, Elizabeth J. and
         {Butler}, Karen and {Calamida}, Annalisa and {Carlberg}, Raymond G. and
         {Carter}, Paul and {Casas}, Ricard and {Castander}, Francisco J. and
         {Choi}, Yumi and {Comparat}, Johan and {Cukanovaite}, Elena and
         {Delubac}, Timoth{\'e}e and {DeVries}, Kaitlin and {Dey}, Sharmila and
         {Dhungana}, Govinda and {Dickinson}, Mark and {Ding}, Zhejie and
         {Donaldson}, John B. and {Duan}, Yutong and
         {Duckworth}, Christopher J. and {Eftekharzadeh}, Sarah and
         {Eisenstein}, Daniel J. and {Etourneau}, Thomas and
         {Fagrelius}, Parker A. and {Farihi}, Jay and {Fitzpatrick}, Mike and
         {Font-Ribera}, Andreu and {Fulmer}, Leah and {G{\"a}nsicke}, Boris T. and
         {Gaztanaga}, Enrique and {George}, Koshy and {Gerdes}, David W. and
         {Gontcho}, Satya Gontcho A. and {Gorgoni}, Claudio and
         {Green}, Gregory and {Guy}, Julien and {Harmer}, Diane and {Hernand
        ez}, M. and {Honscheid}, Klaus and {Huang}, Lijuan Wendy and
         {James}, David J. and {Jannuzi}, Buell T. and {Jiang}, Linhua and
         {Joyce}, Richard and {Karcher}, Armin and {Karkar}, Sonia and
         {Kehoe}, Robert and {Kneib}, Jean-Paul and {Kueter-Young}, Andrea and
         {Lan}, Ting-Wen and {Lauer}, Tod R. and {Le Guillou}, Laurent and
         {Le Van Suu}, Auguste and {Lee}, Jae Hyeon and {Lesser}, Michael and
         {Perreault Levasseur}, Laurence and {Li}, Ting S. and
         {Mann}, Justin L. and {Marshall}, Robert and
         {Mart{\'\i}nez-V{\'a}zquez}, C.~E. and {Martini}, Paul and
         {du Mas des Bourboux}, H{\'e}lion and {McManus}, Sean and
         {Meier}, Tobias Gabriel and {M{\'e}nard}, Brice and {Metcalfe}, Nigel and
         {Mu{\~n}oz-Guti{\'e}rrez}, Andrea and {Najita}, Joan and
         {Napier}, Kevin and {Narayan}, Gautham and {Newman}, Jeffrey A. and
         {Nie}, Jundan and {Nord}, Brian and {Norman}, Dara J. and
         {Olsen}, Knut A.~G. and {Paat}, Anthony and
         {Palanque-Delabrouille}, Nathalie and {Peng}, Xiyan and
         {Poppett}, Claire L. and {Poremba}, Megan R. and {Prakash}, Abhishek and
         {Rabinowitz}, David and {Raichoor}, Anand and {Rezaie}, Mehdi and
         {Robertson}, A.~N. and {Roe}, Natalie A. and {Ross}, Ashley J. and
         {Ross}, Nicholas P. and {Rudnick}, Gregory and {Safonova}, Sasha and
         {Saha}, Abhijit and {S{\'a}nchez}, F. Javier and {Savary}, Elodie and
         {Schweiker}, Heidi and {Scott}, Adam and {Seo}, Hee-Jong and
         {Shan}, Huanyuan and {Silva}, David R. and {Slepian}, Zachary and
         {Soto}, Christian and {Sprayberry}, David and {Staten}, Ryan and
         {Stillman}, Coley M. and {Stupak}, Robert J. and {Summers}, David L. and
         {Sien Tie}, Suk and {Tirado}, H. and {Vargas-Maga{\~n}a}, Mariana and
         {Vivas}, A. Katherina and {Wechsler}, Risa H. and {Williams}, Doug and
         {Yang}, Jinyi and {Yang}, Qian and {Yapici}, Tolga and
         {Zaritsky}, Dennis and {Zenteno}, A. and {Zhang}, Kai and
         {Zhang}, Tianmeng and {Zhou}, Rongpu and {Zhou}, Zhimin},
        title = "{Overview of the DESI Legacy Imaging Surveys}",
      journal = {\aj},
     keywords = {catalogs, surveys, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2019,
        month = may,
       volume = {157},
       number = {5},
          eid = {168},
        pages = {168},
          doi = {10.3847/1538-3881/ab089d},
archivePrefix = {arXiv},
       eprint = {1804.08657},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019AJ....157..168D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Pozzetti2010,
       author = {{Pozzetti}, L. and {Bolzonella}, M. and {Zucca}, E. and {Zamorani}, G. and
         {Lilly}, S. and {Renzini}, A. and {Moresco}, M. and {Mignoli}, M. and
         {Cassata}, P. and {Tasca}, L. and {Lamareille}, F. and {Maier}, C. and
         {Meneux}, B. and {Halliday}, C. and {Oesch}, P. and {Vergani}, D. and
         {Caputi}, K. and {Kova{\v{c}}}, K. and {Cimatti}, A. and
         {Cucciati}, O. and {Iovino}, A. and {Peng}, Y. and {Carollo}, M. and
         {Contini}, T. and {Kneib}, J. -P. and {Le F{\'e}vre}, O. and
         {Mainieri}, V. and {Scodeggio}, M. and {Bardelli}, S. and
         {Bongiorno}, A. and {Coppa}, G. and {de la Torre}, S. and
         {de Ravel}, L. and {Franzetti}, P. and {Garilli}, B. and
         {Kampczyk}, P. and {Knobel}, C. and {Le Borgne}, J. -F. and
         {Le Brun}, V. and {Pell{\`o}}, R. and {Perez Montero}, E. and
         {Ricciardelli}, E. and {Silverman}, J.~D. and {Tanaka}, M. and
         {Tresse}, L. and {Abbas}, U. and {Bottini}, D. and {Cappi}, A. and
         {Guzzo}, L. and {Koekemoer}, A.~M. and {Leauthaud}, A. and
         {Maccagni}, D. and {Marinoni}, C. and {McCracken}, H.~J. and
         {Memeo}, P. and {Porciani}, C. and {Scaramella}, R. and {Scarlata}, C. and
         {Scoville}, N.},
        title = "{zCOSMOS - 10k-bright spectroscopic sample. The bimodality in the galaxy stellar mass function: exploring its evolution with redshift}",
      journal = {\aap},
     keywords = {galaxies: evolution, galaxies: luminosity function, mass function, galaxies:, statistics, galaxies: formation, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2010,
        month = nov,
       volume = {523},
          eid = {A13},
        pages = {A13},
          doi = {10.1051/0004-6361/200913020},
archivePrefix = {arXiv},
       eprint = {0907.5416},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010A&A...523A..13P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Williams2009,
       author = {{Williams}, Rik J. and {Quadri}, Ryan F. and {Franx}, Marijn and
         {van Dokkum}, Pieter and {Labb{\'e}}, Ivo},
        title = "{Detection of Quiescent Galaxies in a Bicolor Sequence from Z = 0-2}",
      journal = {\apj},
     keywords = {cosmology: observations, galaxies: evolution, galaxies: high-redshift, infrared: galaxies, Astrophysics},
         year = 2009,
        month = feb,
       volume = {691},
       number = {2},
        pages = {1879-1895},
          doi = {10.1088/0004-637X/691/2/1879},
archivePrefix = {arXiv},
       eprint = {0806.0625},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009ApJ...691.1879W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Tomczak14,
       author = {{Tomczak}, Adam R. and {Quadri}, Ryan F. and {Tran}, Kim-Vy H. and
         {Labb{\'e}}, Ivo and {Straatman}, Caroline M.~S. and {Papovich}, Casey and
         {Glazebrook}, Karl and {Allen}, Rebecca and {Brammer}, Gabriel B. and
         {Kacprzak}, Glenn G. and {Kawinwanichakij}, Lalitwadee and
         {Kelson}, Daniel D. and {McCarthy}, Patrick J. and {Mehrtens}, Nicola and
         {Monson}, Andrew J. and {Persson}, S. Eric and {Spitler}, Lee R. and
         {Tilvi}, Vithal and {van Dokkum}, Pieter},
        title = "{Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-mass Galaxies since z = 2 and the Rapid Buildup of Quiescent Galaxies}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: high-redshift, galaxies: luminosity function, mass function, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2014,
        month = mar,
       volume = {783},
       number = {2},
          eid = {85},
        pages = {85},
          doi = {10.1088/0004-637X/783/2/85},
archivePrefix = {arXiv},
       eprint = {1309.5972},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014ApJ...783...85T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{arnouts07,
       author = {{Arnouts}, S. and {Walcher}, C.~J. and {Le F{\`e}vre}, O. and {Zamorani}, G. and {Ilbert}, O. and {Le Brun}, V. and {Pozzetti}, L. and {Bardelli}, S. and {Tresse}, L. and {Zucca}, E. and {Charlot}, S. and {Lamareille}, F. and {McCracken}, H.~J. and {Bolzonella}, M. and {Iovino}, A. and {Lonsdale}, C. and {Polletta}, M. and {Surace}, J. and {Bottini}, D. and {Garilli}, B. and {Maccagni}, D. and {Picat}, J.~P. and {Scaramella}, R. and {Scodeggio}, M. and {Vettolani}, G. and {Zanichelli}, A. and {Adami}, C. and {Cappi}, A. and {Ciliegi}, P. and {Contini}, T. and {de la Torre}, S. and {Foucaud}, S. and {Franzetti}, P. and {Gavignaud}, I. and {Guzzo}, L. and {Marano}, B. and {Marinoni}, C. and {Mazure}, A. and {Meneux}, B. and {Merighi}, R. and {Paltani}, S. and {Pell{\`o}}, R. and {Pollo}, A. and {Radovich}, M. and {Temporin}, S. and {Vergani}, D.},
        title = "{The SWIRE-VVDS-CFHTLS surveys: stellar mass assembly over the last 10 Gyr. Evidence for a major build up of the red sequence between z = 2 and z = 1}",
      journal = {\aap},
     keywords = {galaxies: luminosity function, mass function, galaxies: formation, Astrophysics},
         year = 2007,
        month = dec,
       volume = {476},
       number = {1},
        pages = {137-150},
          doi = {10.1051/0004-6361:20077632},
archivePrefix = {arXiv},
       eprint = {0705.2438},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007A&A...476..137A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Moustakas2013,
       author = {{Moustakas}, John and {Coil}, Alison L. and {Aird}, James and
         {Blanton}, Michael R. and {Cool}, Richard J. and
         {Eisenstein}, Daniel J. and {Mendez}, Alexander J. and
         {Wong}, Kenneth C. and {Zhu}, Guangtun and {Arnouts}, St{\'e}phane},
        title = "{PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function from z = 0-1}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: high-redshift, large-scale structure of universe, surveys, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2013,
        month = apr,
       volume = {767},
       number = {1},
          eid = {50},
        pages = {50},
          doi = {10.1088/0004-637X/767/1/50},
archivePrefix = {arXiv},
       eprint = {1301.1688},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJ...767...50M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2019ApJ...887...55C,
       author = {{Casey}, Caitlin M. and {Zavala}, Jorge A. and {Aravena}, Manuel and
         {B{\'e}thermin}, Matthieu and {Caputi}, Karina I. and
         {Champagne}, Jaclyn B. and {Clements}, David L. and
         {da Cunha}, Elisabete and {Drew}, Patrick and {Finkelstein}, Steven L. and
         {Hayward}, Christopher C. and {Kartaltepe}, Jeyhan S. and
         {Knudsen}, Kirsten and {Koekemoer}, Anton M. and {Magdis}, Georgios E. and
         {Man}, Allison and {Manning}, Sinclaire M. and {Scoville}, Nick Z. and
         {Sheth}, Kartik and {Spilker}, Justin and {Staguhn}, Johannes and
         {Talia}, Margherita and {Taniguchi}, Yoshiaki and {Toft}, Sune and
         {Treister}, Ezequiel and {Yun}, Min},
        title = "{Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85}",
      journal = {\apj},
     keywords = {Starburst galaxies, Infrared galaxies, High-redshift galaxies, Blank fields, 1570, 790, 734, 163, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = dec,
       volume = {887},
       number = {1},
          eid = {55},
        pages = {55},
          doi = {10.3847/1538-4357/ab52ff},
archivePrefix = {arXiv},
       eprint = {1910.13331},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...887...55C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2015ApJ...808L..33C,
       author = {{Casey}, C.~M. and {Cooray}, A. and {Capak}, P. and {Fu}, H. and
         {Kovac}, K. and {Lilly}, S. and {Sanders}, D.~B. and {Scoville}, N.~Z. and
         {Treister}, E.},
        title = "{A Massive, Distant Proto-cluster at z = 2.47 Caught in a Phase of Rapid Formation?}",
      journal = {\apjl},
     keywords = {galaxies: clusters: general, galaxies: starburst, large-scale structure of universe, quasars: general, Astrophysics - Astrophysics of Galaxies},
         year = 2015,
        month = aug,
       volume = {808},
       number = {2},
          eid = {L33},
        pages = {L33},
          doi = {10.1088/2041-8205/808/2/L33},
archivePrefix = {arXiv},
       eprint = {1506.01715},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015ApJ...808L..33C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2016ApJ...826..130H,
       author = {{Hung}, Chao-Ling and {Casey}, Caitlin M. and {Chiang}, Yi-Kuan and
         {Capak}, Peter L. and {Cowley}, Michael J. and {Darvish}, Behnam and
         {Kacprzak}, Glenn G. and {Kova{\v{c}}}, K. and {Lilly}, Simon J. and
         {Nanayakkara}, Themiya and {Spitler}, Lee R. and {Tran}, Kim-Vy H. and
         {Yuan}, Tiantian},
        title = "{Large-scale Structure around a z=2.1 Cluster}",
      journal = {\apj},
     keywords = {galaxies: clusters: general, galaxies: starburst, large-scale structure of universe, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = aug,
       volume = {826},
       number = {2},
          eid = {130},
        pages = {130},
          doi = {10.3847/0004-637X/826/2/130},
archivePrefix = {arXiv},
       eprint = {1605.07176},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016ApJ...826..130H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2006astro.ph..9591A,
       author = {{Albrecht}, Andreas and {Bernstein}, Gary and {Cahn}, Robert and
         {Freedman}, Wendy L. and {Hewitt}, Jacqueline and {Hu}, Wayne and
         {Huth}, John and {Kamionkowski}, Marc and {Kolb}, Edward W. and
         {Knox}, Lloyd and {Mather}, John C. and {Staggs}, Suzanne and
         {Suntzeff}, Nicholas B.},
        title = "{Report of the Dark Energy Task Force}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics},
         year = 2006,
        month = sep,
          eid = {astro-ph/0609591},
        pages = {astro-ph/0609591},
archivePrefix = {arXiv},
       eprint = {astro-ph/0609591},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2006astro.ph..9591A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2013A&A...558A..67A,
       author = {{Arnouts}, S. and {Le Floc'h}, E. and {Chevallard}, J. and
         {Johnson}, B.~D. and {Ilbert}, O. and {Treyer}, M. and {Aussel}, H. and
         {Capak}, P. and {Sanders}, D.~B. and {Scoville}, N. and
         {McCracken}, H.~J. and {Milliard}, B. and {Pozzetti}, L. and
         {Salvato}, M.},
        title = "{Encoding of the infrared excess in the NUVrK color diagram for star-forming galaxies}",
      journal = {\aap},
     keywords = {infrared: galaxies, ultraviolet: galaxies, galaxies: evolution, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = oct,
       volume = {558},
          eid = {A67},
        pages = {A67},
          doi = {10.1051/0004-6361/201321768},
archivePrefix = {arXiv},
       eprint = {1309.0008},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013A&A...558A..67A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2017ApJS..228....7N,
       author = {{Nayyeri}, H. and {Hemmati}, S. and {Mobasher}, B. and
         {Ferguson}, H.~C. and {Cooray}, A. and {Barro}, G. and {Faber}, S.~M. and
         {Dickinson}, M. and {Koekemoer}, A.~M. and {Peth}, M. and
         {Salvato}, M. and {Ashby}, M.~L.~N. and {Darvish}, B. and {Donley}, J. and
         {Durbin}, M. and {Finkelstein}, S. and {Fontana}, A. and
         {Grogin}, N.~A. and {Gruetzbauch}, R. and {Huang}, K. and
         {Khostovan}, A.~A. and {Kocevski}, D. and {Kodra}, D. and {Lee}, B. and
         {Newman}, J. and {Pacifici}, C. and {Pforr}, J. and {Stefanon}, M. and
         {Wiklind}, T. and {Willner}, S.~P. and {Wuyts}, S. and
         {Castellano}, M. and {Conselice}, C. and {Dolch}, T. and
         {Dunlop}, J.~S. and {Galametz}, A. and {Hathi}, N.~P. and
         {Lucas}, R.~A. and {Yan}, H.},
        title = "{CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field}",
      journal = {\apjs},
     keywords = {catalogs, galaxies: high-redshift, galaxies: photometry, methods: data analysis, techniques: image processing, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = jan,
       volume = {228},
       number = {1},
          eid = {7},
        pages = {7},
          doi = {10.3847/1538-4365/228/1/7},
archivePrefix = {arXiv},
       eprint = {1612.07364},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017ApJS..228....7N},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2009ApJ...699..486C,
       author = {{Conroy}, Charlie and {Gunn}, James E. and {White}, Martin},
        title = "{The Propagation of Uncertainties in Stellar Population Synthesis Modeling. I. The Relevance of Uncertain Aspects of Stellar Evolution and the Initial Mass Function to the Derived Physical Properties of Galaxies}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: stellar content, stars: evolution, Astrophysics},
         year = 2009,
        month = jul,
       volume = {699},
       number = {1},
        pages = {486-506},
          doi = {10.1088/0004-637X/699/1/486},
archivePrefix = {arXiv},
       eprint = {0809.4261},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009ApJ...699..486C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2010ApJ...712..833C,
       author = {{Conroy}, Charlie and {Gunn}, James E.},
        title = "{The Propagation of Uncertainties in Stellar Population Synthesis Modeling. III. Model Calibration, Comparison, and Evaluation}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: stellar content, stars: evolution, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2010,
        month = apr,
       volume = {712},
       number = {2},
        pages = {833-857},
          doi = {10.1088/0004-637X/712/2/833},
archivePrefix = {arXiv},
       eprint = {0911.3151},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010ApJ...712..833C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2008PASP..120..212G,
       author = {{Gwyn}, Stephen D.~J.},
        title = "{MegaPipe: The MegaCam Image Stacking Pipeline at the Canadian Astronomical Data Centre}",
      journal = {\pasp},
     keywords = {Astrophysics},
         year = 2008,
        month = feb,
       volume = {120},
       number = {864},
        pages = {212},
          doi = {10.1086/526794},
archivePrefix = {arXiv},
       eprint = {0710.0370},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2008PASP..120..212G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Aihara_2011,
       author = {{Aihara}, Hiroaki and {Allende Prieto}, Carlos and {An}, Deokkeun and
         {Anderson}, Scott F. and {Aubourg}, {\'E}ric and {Balbinot}, Eduardo and
         {Beers}, Timothy C. and {Berlind}, Andreas A. and
         {Bickerton}, Steven J. and {Bizyaev}, Dmitry and {Blanton}, Michael R. and
         {Bochanski}, John J. and {Bolton}, Adam S. and {Bovy}, Jo and {Brand
        t}, W.~N. and {Brinkmann}, J. and {Brown}, Peter J. and
         {Brownstein}, Joel R. and {Busca}, Nicolas G. and {Campbell}, Heather and
         {Carr}, Michael A. and {Chen}, Yanmei and {Chiappini}, Cristina and
         {Comparat}, Johan and {Connolly}, Natalia and {Cortes}, Marina and
         {Croft}, Rupert A.~C. and {Cuesta}, Antonio J. and {da Costa}, Luiz N. and
         {Davenport}, James R.~A. and {Dawson}, Kyle and {Dhital}, Saurav and
         {Ealet}, Anne and {Ebelke}, Garrett L. and {Edmondson}, Edward M. and
         {Eisenstein}, Daniel J. and {Escoffier}, Stephanie and
         {Esposito}, Massimiliano and {Evans}, Michael L. and {Fan}, Xiaohui and
         {Femen{\'\i}a Castell{\'a}}, Bruno and {Font-Ribera}, Andreu and
         {Frinchaboy}, Peter M. and {Ge}, Jian and {Gillespie}, Bruce A. and
         {Gilmore}, G. and {Gonz{\'a}lez Hern{\'a}ndez}, Jonay I. and
         {Gott}, J. Richard and {Gould}, Andrew and {Grebel}, Eva K. and
         {Gunn}, James E. and {Hamilton}, Jean-Christophe and {Harding}, Paul and
         {Harris}, David W. and {Hawley}, Suzanne L. and {Hearty}, Frederick R. and
         {Ho}, Shirley and {Hogg}, David W. and {Holtzman}, Jon A. and
         {Honscheid}, Klaus and {Inada}, Naohisa and {Ivans}, Inese I. and
         {Jiang}, Linhua and {Johnson}, Jennifer A. and {Jordan}, Cathy and
         {Jordan}, Wendell P. and {Kazin}, Eyal A. and {Kirkby}, David and
         {Klaene}, Mark A. and {Knapp}, G.~R. and {Kneib}, Jean-Paul and
         {Kochanek}, C.~S. and {Koesterke}, Lars and {Kollmeier}, Juna A. and
         {Kron}, Richard G. and {Lampeitl}, Hubert and {Lang}, Dustin and
         {Le Goff}, Jean-Marc and {Lee}, Young Sun and {Lin}, Yen-Ting and
         {Long}, Daniel C. and {Loomis}, Craig P. and {Lucatello}, Sara and
         {Lundgren}, Britt and {Lupton}, Robert H. and {Ma}, Zhibo and
         {MacDonald}, Nicholas and {Mahadevan}, Suvrath and
         {Maia}, Marcio A.~G. and {Makler}, Martin and {Malanushenko}, Elena and
         {Malanushenko}, Viktor and {Mandelbaum}, Rachel and
         {Maraston}, Claudia and {Margala}, Daniel and {Masters}, Karen L. and
         {McBride}, Cameron K. and {McGehee}, Peregrine M. and
         {McGreer}, Ian D. and {M{\'e}nard}, Brice and
         {Miralda-Escud{\'e}}, Jordi and {Morrison}, Heather L. and
         {Mullally}, F. and {Muna}, Demitri and {Munn}, Jeffrey A. and
         {Murayama}, Hitoshi and {Myers}, Adam D. and {Naugle}, Tracy and
         {Neto}, Angelo Fausti and {Nguyen}, Duy Cuong and {Nichol}, Robert C. and
         {O'Connell}, Robert W. and {Ogando}, Ricardo L.~C. and
         {Olmstead}, Matthew D. and {Oravetz}, Daniel J. and
         {Padmanabhan}, Nikhil and {Palanque-Delabrouille}, Nathalie and
         {Pan}, Kaike and {Pandey}, Parul and {P{\^a}ris}, Isabelle and
         {Percival}, Will J. and {Petitjean}, Patrick and
         {Pfaffenberger}, Robert and {Pforr}, Janine and {Phleps}, Stefanie and
         {Pichon}, Christophe and {Pieri}, Matthew M. and {Prada}, Francisco and
         {Price-Whelan}, Adrian M. and {Raddick}, M. Jordan and
         {Ramos}, Beatriz H.~F. and {Reyl{\'e}}, C{\'e}line and {Rich}, James and
         {Richards}, Gordon T. and {Rix}, Hans-Walter and {Robin}, Annie C. and
         {Rocha-Pinto}, Helio J. and {Rockosi}, Constance M. and
         {Roe}, Natalie A. and {Rollinde}, Emmanuel and {Ross}, Ashley J. and
         {Ross}, Nicholas P. and {Rossetto}, Bruno M. and
         {S{\'a}nchez}, Ariel G. and {Sayres}, Conor and {Schlegel}, David J. and
         {Schlesinger}, Katharine J. and {Schmidt}, Sarah J. and
         {Schneider}, Donald P. and {Sheldon}, Erin and {Shu}, Yiping and
         {Simmerer}, Jennifer and {Simmons}, Audrey E. and
         {Sivarani}, Thirupathi and {Snedden}, Stephanie A. and
         {Sobeck}, Jennifer S. and {Steinmetz}, Matthias and
         {Strauss}, Michael A. and {Szalay}, Alexander S. and
         {Tanaka}, Masayuki and {Thakar}, Aniruddha R. and {Thomas}, Daniel and
         {Tinker}, Jeremy L. and {Tofflemire}, Benjamin M. and {Tojeiro}, Rita and
         {Tremonti}, Christy A. and {Vandenberg}, Jan and
         {Vargas Maga{\~n}a}, M. and {Verde}, Licia and {Vogt}, Nicole P. and
         {Wake}, David A. and {Wang}, Ji and {Weaver}, Benjamin A. and
         {Weinberg}, David H. and {White}, Martin and {White}, Simon D.~M. and
         {Yanny}, Brian and {Yasuda}, Naoki and {Yeche}, Christophe and
         {Zehavi}, Idit},
        title = "{The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III}",
      journal = {\apjs},
     keywords = {atlases, catalogs, surveys, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2011,
        month = apr,
       volume = {193},
       number = {2},
          eid = {29},
        pages = {29},
          doi = {10.1088/0067-0049/193/2/29},
archivePrefix = {arXiv},
       eprint = {1101.1559},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJS..193...29A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Madau_2014,
       author = {{Madau}, Piero and {Dickinson}, Mark},
        title = "{Cosmic Star-Formation History}",
      journal = {\araa},
     keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2014,
        month = aug,
       volume = {52},
        pages = {415-486},
          doi = {10.1146/annurev-astro-081811-125615},
archivePrefix = {arXiv},
       eprint = {1403.0007},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014ARA&A..52..415M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Giavalisco_2004,
       author = {{Giavalisco}, M. and {Ferguson}, H.~C. and {Koekemoer}, A.~M. and
         {Dickinson}, M. and {Alexander}, D.~M. and {Bauer}, F.~E. and
         {Bergeron}, J. and {Biagetti}, C. and {Brandt}, W.~N. and
         {Casertano}, S. and {Cesarsky}, C. and {Chatzichristou}, E. and
         {Conselice}, C. and {Cristiani}, S. and {Da Costa}, L. and
         {Dahlen}, T. and {de Mello}, D. and {Eisenhardt}, P. and {Erben}, T. and
         {Fall}, S.~M. and {Fassnacht}, C. and {Fosbury}, R. and {Fruchter}, A. and
         {Gardner}, J.~P. and {Grogin}, N. and {Hook}, R.~N. and
         {Hornschemeier}, A.~E. and {Idzi}, R. and {Jogee}, S. and
         {Kretchmer}, C. and {Laidler}, V. and {Lee}, K.~S. and {Livio}, M. and
         {Lucas}, R. and {Madau}, P. and {Mobasher}, B. and {Moustakas}, L.~A. and
         {Nonino}, M. and {Padovani}, P. and {Papovich}, C. and {Park}, Y. and
         {Ravindranath}, S. and {Renzini}, A. and {Richardson}, M. and
         {Riess}, A. and {Rosati}, P. and {Schirmer}, M. and {Schreier}, E. and
         {Somerville}, R.~S. and {Spinrad}, H. and {Stern}, D. and
         {Stiavelli}, M. and {Strolger}, L. and {Urry}, C.~M. and {Vandame}, B. and
         {Williams}, R. and {Wolf}, C.},
        title = "{The Great Observatories Origins Deep Survey: Initial Results from Optical and Near-Infrared Imaging}",
      journal = {\apjl},
     keywords = {Cosmology: Observations, Galaxies: Distances and Redshifts, Galaxies: Evolution, Galaxies: Formation, Astrophysics},
         year = 2004,
        month = jan,
       volume = {600},
       number = {2},
        pages = {L93-L98},
          doi = {10.1086/379232},
archivePrefix = {arXiv},
       eprint = {astro-ph/0309105},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2004ApJ...600L..93G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Beckwith_2006,
       author = {{Beckwith}, Steven V.~W. and {Stiavelli}, Massimo and
         {Koekemoer}, Anton M. and {Caldwell}, John A.~R. and
         {Ferguson}, Henry C. and {Hook}, Richard and {Lucas}, Ray A. and
         {Bergeron}, Louis E. and {Corbin}, Michael and {Jogee}, Shardha and
         {Panagia}, Nino and {Robberto}, Massimo and {Royle}, Patricia and
         {Somerville}, Rachel S. and {Sosey}, Megan},
        title = "{The Hubble Ultra Deep Field}",
      journal = {\aj},
     keywords = {Astronomical Data Bases: Miscellaneous, Cosmology: Early Universe, Galaxies: Evolution, Galaxies: High-Redshift, Astrophysics},
         year = 2006,
        month = nov,
       volume = {132},
       number = {5},
        pages = {1729-1755},
          doi = {10.1086/507302},
archivePrefix = {arXiv},
       eprint = {astro-ph/0607632},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2006AJ....132.1729B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Grogin_2011,
       author = {{Grogin}, Norman A. and {Kocevski}, Dale D. and {Faber}, S.~M. and
         {Ferguson}, Henry C. and {Koekemoer}, Anton M. and {Riess}, Adam G. and
         {Acquaviva}, Viviana and {Alexander}, David M. and {Almaini}, Omar and
         {Ashby}, Matthew L.~N. and {Barden}, Marco and {Bell}, Eric F. and
         {Bournaud}, Fr{\'e}d{\'e}ric and {Brown}, Thomas M. and
         {Caputi}, Karina I. and {Casertano}, Stefano and {Cassata}, Paolo and
         {Castellano}, Marco and {Challis}, Peter and {Chary}, Ranga-Ram and
         {Cheung}, Edmond and {Cirasuolo}, Michele and
         {Conselice}, Christopher J. and {Roshan Cooray}, Asantha and
         {Croton}, Darren J. and {Daddi}, Emanuele and {Dahlen}, Tomas and
         {Dav{\'e}}, Romeel and {de Mello}, Du{\'\i}lia F. and {Dekel}, Avishai and
         {Dickinson}, Mark and {Dolch}, Timothy and {Donley}, Jennifer L. and
         {Dunlop}, James S. and {Dutton}, Aaron A. and {Elbaz}, David and
         {Fazio}, Giovanni G. and {Filippenko}, Alexei V. and
         {Finkelstein}, Steven L. and {Fontana}, Adriano and
         {Gardner}, Jonathan P. and {Garnavich}, Peter M. and {Gawiser}, Eric and
         {Giavalisco}, Mauro and {Grazian}, Andrea and {Guo}, Yicheng and
         {Hathi}, Nimish P. and {H{\"a}ussler}, Boris and {Hopkins}, Philip F. and
         {Huang}, Jia-Sheng and {Huang}, Kuang-Han and {Jha}, Saurabh W. and
         {Kartaltepe}, Jeyhan S. and {Kirshner}, Robert P. and {Koo}, David C. and
         {Lai}, Kamson and {Lee}, Kyoung-Soo and {Li}, Weidong and
         {Lotz}, Jennifer M. and {Lucas}, Ray A. and {Madau}, Piero and
         {McCarthy}, Patrick J. and {McGrath}, Elizabeth J. and
         {McIntosh}, Daniel H. and {McLure}, Ross J. and {Mobasher}, Bahram and
         {Moustakas}, Leonidas A. and {Mozena}, Mark and {Nandra}, Kirpal and
         {Newman}, Jeffrey A. and {Niemi}, Sami-Matias and {Noeske}, Kai G. and
         {Papovich}, Casey J. and {Pentericci}, Laura and {Pope}, Alexandra and
         {Primack}, Joel R. and {Rajan}, Abhijith and {Ravindranath}, Swara and
         {Reddy}, Naveen A. and {Renzini}, Alvio and {Rix}, Hans-Walter and
         {Robaina}, Aday R. and {Rodney}, Steven A. and {Rosario}, David J. and
         {Rosati}, Piero and {Salimbeni}, Sara and {Scarlata}, Claudia and
         {Siana}, Brian and {Simard}, Luc and {Smidt}, Joseph and
         {Somerville}, Rachel S. and {Spinrad}, Hyron and {Straughn}, Amber N. and
         {Strolger}, Louis-Gregory and {Telford}, Olivia and
         {Teplitz}, Harry I. and {Trump}, Jonathan R. and {van der Wel}, Arjen and
         {Villforth}, Carolin and {Wechsler}, Risa H. and {Weiner}, Benjamin J. and
         {Wiklind}, Tommy and {Wild}, Vivienne and {Wilson}, Grant and
         {Wuyts}, Stijn and {Yan}, Hao-Jing and {Yun}, Min S.},
        title = "{CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey}",
      journal = {\apjs},
     keywords = {cosmology: observations, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2011,
        month = dec,
       volume = {197},
       number = {2},
          eid = {35},
        pages = {35},
          doi = {10.1088/0067-0049/197/2/35},
archivePrefix = {arXiv},
       eprint = {1105.3753},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJS..197...35G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Koekemoer_2011,
       author = {{Koekemoer}, Anton M. and {Faber}, S.~M. and {Ferguson}, Henry C. and
         {Grogin}, Norman A. and {Kocevski}, Dale D. and {Koo}, David C. and
         {Lai}, Kamson and {Lotz}, Jennifer M. and {Lucas}, Ray A. and
         {McGrath}, Elizabeth J. and {Ogaz}, Sara and {Rajan}, Abhijith and
         {Riess}, Adam G. and {Rodney}, Steve A. and {Strolger}, Louis and
         {Casertano}, Stefano and {Castellano}, Marco and {Dahlen}, Tomas and
         {Dickinson}, Mark and {Dolch}, Timothy and {Fontana}, Adriano and
         {Giavalisco}, Mauro and {Grazian}, Andrea and {Guo}, Yicheng and
         {Hathi}, Nimish P. and {Huang}, Kuang-Han and {van der Wel}, Arjen and
         {Yan}, Hao-Jing and {Acquaviva}, Viviana and {Alexander}, David M. and
         {Almaini}, Omar and {Ashby}, Matthew L.~N. and {Barden}, Marco and
         {Bell}, Eric F. and {Bournaud}, Fr{\'e}d{\'e}ric and
         {Brown}, Thomas M. and {Caputi}, Karina I. and {Cassata}, Paolo and
         {Challis}, Peter J. and {Chary}, Ranga-Ram and {Cheung}, Edmond and
         {Cirasuolo}, Michele and {Conselice}, Christopher J. and
         {Roshan Cooray}, Asantha and {Croton}, Darren J. and {Daddi}, Emanuele and
         {Dav{\'e}}, Romeel and {de Mello}, Duilia F. and {de Ravel}, Loic and
         {Dekel}, Avishai and {Donley}, Jennifer L. and {Dunlop}, James S. and
         {Dutton}, Aaron A. and {Elbaz}, David and {Fazio}, Giovanni G. and
         {Filippenko}, Alexei V. and {Finkelstein}, Steven L. and
         {Frazer}, Chris and {Gardner}, Jonathan P. and {Garnavich}, Peter M. and
         {Gawiser}, Eric and {Gruetzbauch}, Ruth and {Hartley}, Will G. and
         {H{\"a}ussler}, Boris and {Herrington}, Jessica and
         {Hopkins}, Philip F. and {Huang}, Jia-Sheng and {Jha}, Saurabh W. and
         {Johnson}, Andrew and {Kartaltepe}, Jeyhan S. and {Khostovan}, Ali A. and
         {Kirshner}, Robert P. and {Lani}, Caterina and {Lee}, Kyoung-Soo and
         {Li}, Weidong and {Madau}, Piero and {McCarthy}, Patrick J. and
         {McIntosh}, Daniel H. and {McLure}, Ross J. and {McPartland}, Conor and
         {Mobasher}, Bahram and {Moreira}, Heidi and {Mortlock}, Alice and
         {Moustakas}, Leonidas A. and {Mozena}, Mark and {Nandra}, Kirpal and
         {Newman}, Jeffrey A. and {Nielsen}, Jennifer L. and {Niemi}, Sami and
         {Noeske}, Kai G. and {Papovich}, Casey J. and {Pentericci}, Laura and
         {Pope}, Alexandra and {Primack}, Joel R. and {Ravindranath}, Swara and
         {Reddy}, Naveen A. and {Renzini}, Alvio and {Rix}, Hans-Walter and
         {Robaina}, Aday R. and {Rosario}, David J. and {Rosati}, Piero and
         {Salimbeni}, Sara and {Scarlata}, Claudia and {Siana}, Brian and
         {Simard}, Luc and {Smidt}, Joseph and {Snyder}, Diana and
         {Somerville}, Rachel S. and {Spinrad}, Hyron and {Straughn}, Amber N. and
         {Telford}, Olivia and {Teplitz}, Harry I. and {Trump}, Jonathan R. and
         {Vargas}, Carlos and {Villforth}, Carolin and {Wagner}, Cory R. and {Wand
        ro}, Pat and {Wechsler}, Risa H. and {Weiner}, Benjamin J. and
         {Wiklind}, Tommy and {Wild}, Vivienne and {Wilson}, Grant and
         {Wuyts}, Stijn and {Yun}, Min S.},
        title = "{CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey{\textemdash}The Hubble Space Telescope Observations, Imaging Data Products, and Mosaics}",
      journal = {\apjs},
     keywords = {cosmology: observations, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2011,
        month = dec,
       volume = {197},
       number = {2},
          eid = {36},
        pages = {36},
          doi = {10.1088/0067-0049/197/2/36},
archivePrefix = {arXiv},
       eprint = {1105.3754},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJS..197...36K},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@article{astropy1,
  Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
  Adsurl = {http://adsabs.harvard.edu/abs/2013A%26A...558A..33A},
  Archiveprefix = {arXiv},
  Author = {{Astropy Collaboration} and {Robitaille}, T.~P. and {Tollerud}, E.~J. and {Greenfield}, P. and {Droettboom}, M. and {Bray}, E. and {Aldcroft}, T. and {Davis}, M. and {Ginsburg}, A. and {Price-Whelan}, A.~M. and {Kerzendorf}, W.~E. and {Conley}, A. and {Crighton}, N. and {Barbary}, K. and {Muna}, D. and {Ferguson}, H. and {Grollier}, F. and {Parikh}, M.~M. and {Nair}, P.~H. and {Unther}, H.~M. and {Deil}, C. and {Woillez}, J. and {Conseil}, S. and {Kramer}, R. and {Turner}, J.~E.~H. and {Singer}, L. and {Fox}, R. and {Weaver}, B.~A. and {Zabalza}, V. and {Edwards}, Z.~I. and {Azalee Bostroem}, K. and {Burke}, D.~J. and {Casey}, A.~R. and {Crawford}, S.~M. and {Dencheva}, N. and {Ely}, J. and {Jenness}, T. and {Labrie}, K. and {Lim}, P.~L. and {Pierfederici}, F. and {Pontzen}, A. and {Ptak}, A. and {Refsdal}, B. and {Servillat}, M. and {Streicher}, O.},
  Doi = {10.1051/0004-6361/201322068},
  Eid = {A33},
  Eprint = {1307.6212},
  Journal = {\aap},
  Keywords = {methods: data analysis, methods: miscellaneous, virtual observatory tools},
  Month = oct,
  Pages = {A33},
  Primaryclass = {astro-ph.IM},
  Title = {{Astropy: A community Python package for astronomy}},
  Volume = 558,
  Year = 2013,
  Bdsk-Url-1 = {https://dx.doi.org/10.1051/0004-6361/201322068}}
@article{astropy2,
  Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
  Adsurl = {https://ui.adsabs.harvard.edu/#abs/2018AJ....156..123T},
  Author = {{Price-Whelan}, A.~M. and {Sip{\H{o}}cz}, B.~M. and {G{\"u}nther}, H.~M. and {Lim}, P.~L. and {Crawford}, S.~M. and {Conseil}, S. and {Shupe}, D.~L. and {Craig}, M.~W. and {Dencheva}, N. and {Ginsburg}, A. and {VanderPlas}, J.~T. and {Bradley}, L.~D. and {P{\'e}rez-Su{\'a}rez}, D. and {de Val-Borro}, M. and {Paper Contributors}, (Primary and {Aldcroft}, T.~L. and {Cruz}, K.~L. and {Robitaille}, T.~P. and {Tollerud}, E.~J. and {Coordination Committee}, (Astropy and {Ardelean}, C. and {Babej}, T. and {Bach}, Y.~P. and {Bachetti}, M. and {Bakanov}, A.~V. and {Bamford}, S.~P. and {Barentsen}, G. and {Barmby}, P. and {Baumbach}, A. and {Berry}, K.~L. and {Biscani}, F. and {Boquien}, M. and {Bostroem}, K.~A. and {Bouma}, L.~G. and {Brammer}, G.~B. and {Bray}, E.~M. and {Breytenbach}, H. and {Buddelmeijer}, H. and {Burke}, D.~J. and {Calderone}, G. and {Cano Rodr{\'\i}guez}, J.~L. and {Cara}, M. and {Cardoso}, J.~V.~M. and {Cheedella}, S. and {Copin}, Y. and {Corrales}, L. and {Crichton}, D. and {D{\textquoteright}Avella}, D. and {Deil}, C. and {Depagne}, {\'E}. and {Dietrich}, J.~P. and {Donath}, A. and {Droettboom}, M. and {Earl}, N. and {Erben}, T. and {Fabbro}, S. and {Ferreira}, L.~A. and {Finethy}, T. and {Fox}, R.~T. and {Garrison}, L.~H. and {Gibbons}, S.~L.~J. and {Goldstein}, D.~A. and {Gommers}, R. and {Greco}, J.~P. and {Greenfield}, P. and {Groener}, A.~M. and {Grollier}, F. and {Hagen}, A. and {Hirst}, P. and {Homeier}, D. and {Horton}, A.~J. and {Hosseinzadeh}, G. and {Hu}, L. and {Hunkeler}, J.~S. and {Ivezi{\'c}}, {\v{Z}}. and {Jain}, A. and {Jenness}, T. and {Kanarek}, G. and {Kendrew}, S. and {Kern}, N.~S. and {Kerzendorf}, W.~E. and {Khvalko}, A. and {King}, J. and {Kirkby}, D. and {Kulkarni}, A.~M. and {Kumar}, A. and {Lee}, A. and {Lenz}, D. and {Littlefair}, S.~P. and {Ma}, Z. and {Macleod}, D.~M. and {Mastropietro}, M. and {McCully}, C. and {Montagnac}, S. and {Morris}, B.~M. and {Mueller}, M. and {Mumford}, S.~J. and {Muna}, D. and {Murphy}, N.~A. and {Nelson}, S. and {Nguyen}, G.~H. and {Ninan}, J.~P. and {N{\"o}the}, M. and {Ogaz}, S. and {Oh}, S. and {Parejko}, J.~K. and {Parley}, N. and {Pascual}, S. and {Patil}, R. and {Patil}, A.~A. and {Plunkett}, A.~L. and {Prochaska}, J.~X. and {Rastogi}, T. and {Reddy Janga}, V. and {Sabater}, J. and {Sakurikar}, P. and {Seifert}, M. and {Sherbert}, L.~E. and {Sherwood-Taylor}, H. and {Shih}, A.~Y. and {Sick}, J. and {Silbiger}, M.~T. and {Singanamalla}, S. and {Singer}, L.~P. and {Sladen}, P.~H. and {Sooley}, K.~A. and {Sornarajah}, S. and {Streicher}, O. and {Teuben}, P. and {Thomas}, S.~W. and {Tremblay}, G.~R. and {Turner}, J.~E.~H. and {Terr{\'o}n}, V. and {van Kerkwijk}, M.~H. and {de la Vega}, A. and {Watkins}, L.~L. and {Weaver}, B.~A. and {Whitmore}, J.~B. and {Woillez}, J. and {Zabalza}, V. and {Contributors}, (Astropy},
  Doi = {10.3847/1538-3881/aabc4f},
  Eid = {123},
  Journal = {\aj},
  Keywords = {methods: data analysis, methods: miscellaneous, methods: statistical, reference systems, Astrophysics - Instrumentation and Methods for Astrophysics},
  Month = Sep,
  Pages = {123},
  Primaryclass = {astro-ph.IM},
  Title = {{The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package}},
  Volume = {156},
  Year = 2018,
  Bdsk-Url-1 = {https://doi.org/10.3847/1538-3881/aabc4f}}
@article{matplotlib,
  Author    = {Hunter, J. D.},
  Title     = {Matplotlib: A 2D graphics environment},
  Journal   = {Computing in Science \& Engineering},
  Volume    = {9},
  Number    = {3},
  Pages     = {90--95},
  abstract  = {Matplotlib is a 2D graphics package used for Python for
  application development, interactive scripting, and publication-quality
  image generation across user interfaces and operating systems.},
  publisher = {IEEE COMPUTER SOC},
  doi       = {10.1109/MCSE.2007.55},
  year      = 2007
}
@article{numpy,
  author={S. {van der Walt} and S. C. {Colbert} and G. {Varoquaux}},
  doi={10.1109/MCSE.2011.37},
  journal={Computing in Science Engineering},
  title={The NumPy Array: A Structure for Efficient Numerical Computation},
  year={2011},
  volume={13},
  number={2},
  pages={22-30},}
@book{python,
  author = {Van Rossum, Guido and Drake, Fred L.},
  title = {Python 3 Reference Manual},
  year = {2009},
  isbn = {1441412697},
  publisher = {CreateSpace},
  address = {Scotts Valley, CA}
}
@article{scipy,
  author = {{Virtanen}, Pauli and {Gommers}, Ralf and {Oliphant},
     Travis E. and {Haberland}, Matt and {Reddy}, Tyler and
     {Cournapeau}, David and {Burovski}, Evgeni and {Peterson}, Pearu
     and {Weckesser}, Warren and {Bright}, Jonathan and {van der Walt},
     St{\'e}fan J.  and {Brett}, Matthew and {Wilson}, Joshua and
     {Jarrod Millman}, K.  and {Mayorov}, Nikolay and {Nelson}, Andrew
     R.~J. and {Jones}, Eric and {Kern}, Robert and {Larson}, Eric and
     {Carey}, CJ and {Polat}, {\.I}lhan and {Feng}, Yu and {Moore},
     Eric W. and {Vand erPlas}, Jake and {Laxalde}, Denis and
     {Perktold}, Josef and {Cimrman}, Robert and {Henriksen}, Ian and
     {Quintero}, E.~A. and {Harris}, Charles R and {Archibald}, Anne M.
     and {Ribeiro}, Ant{\^o}nio H. and {Pedregosa}, Fabian and
     {van Mulbregt}, Paul and {Contributors}, SciPy 1. 0},
    title = "{SciPy 1.0: Fundamental Algorithms for Scientific
              Computing in Python}",
  journal = {Nature Methods},
  year = "2020",
  volume={17},
  pages={261--272},
  adsurl = {https://rdcu.be/b08Wh},
  doi = {10.1038/s41592-019-0686-2},
}

@ARTICLE{EuclidRedBook,
       author = {{Laureijs}, R. and {Amiaux}, J. and {Arduini}, S. and {Augu{\`e}res}, J. -L. and {Brinchmann}, J. and {Cole}, R. and {Cropper}, M. and {Dabin}, C. and {Duvet}, L. and {Ealet}, A. and {Garilli}, B. and {Gondoin}, P. and {Guzzo}, L. and {Hoar}, J. and {Hoekstra}, H. and {Holmes}, R. and {Kitching}, T. and {Maciaszek}, T. and {Mellier}, Y. and {Pasian}, F. and {Percival}, W. and {Rhodes}, J. and {Saavedra Criado}, G. and {Sauvage}, M. and {Scaramella}, R. and {Valenziano}, L. and {Warren}, S. and {Bender}, R. and {Castander}, F. and {Cimatti}, A. and {Le F{\`e}vre}, O. and {Kurki-Suonio}, H. and {Levi}, M. and {Lilje}, P. and {Meylan}, G. and {Nichol}, R. and {Pedersen}, K. and {Popa}, V. and {Rebolo Lopez}, R. and {Rix}, H. -W. and {Rottgering}, H. and {Zeilinger}, W. and {Grupp}, F. and {Hudelot}, P. and {Massey}, R. and {Meneghetti}, M. and {Miller}, L. and {Paltani}, S. and {Paulin-Henriksson}, S. and {Pires}, S. and {Saxton}, C. and {Schrabback}, T. and {Seidel}, G. and {Walsh}, J. and {Aghanim}, N. and {Amendola}, L. and {Bartlett}, J. and {Baccigalupi}, C. and {Beaulieu}, J. -P. and {Benabed}, K. and {Cuby}, J. -G. and {Elbaz}, D. and {Fosalba}, P. and {Gavazzi}, G. and {Helmi}, A. and {Hook}, I. and {Irwin}, M. and {Kneib}, J. -P. and {Kunz}, M. and {Mannucci}, F. and {Moscardini}, L. and {Tao}, C. and {Teyssier}, R. and {Weller}, J. and {Zamorani}, G. and {Zapatero Osorio}, M.~R. and {Boulade}, O. and {Foumond}, J.~J. and {Di Giorgio}, A. and {Guttridge}, P. and {James}, A. and {Kemp}, M. and {Martignac}, J. and {Spencer}, A. and {Walton}, D. and {Bl{\"u}mchen}, T. and {Bonoli}, C. and {Bortoletto}, F. and {Cerna}, C. and {Corcione}, L. and {Fabron}, C. and {Jahnke}, K. and {Ligori}, S. and {Madrid}, F. and {Martin}, L. and {Morgante}, G. and {Pamplona}, T. and {Prieto}, E. and {Riva}, M. and {Toledo}, R. and {Trifoglio}, M. and {Zerbi}, F. and {Abdalla}, F. and {Douspis}, M. and {Grenet}, C. and {Borgani}, S. and {Bouwens}, R. and {Courbin}, F. and {Delouis}, J. -M. and {Dubath}, P. and {Fontana}, A. and {Frailis}, M. and {Grazian}, A. and {Koppenh{\"o}fer}, J. and {Mansutti}, O. and {Melchior}, M. and {Mignoli}, M. and {Mohr}, J. and {Neissner}, C. and {Noddle}, K. and {Poncet}, M. and {Scodeggio}, M. and {Serrano}, S. and {Shane}, N. and {Starck}, J. -L. and {Surace}, C. and {Taylor}, A. and {Verdoes-Kleijn}, G. and {Vuerli}, C. and {Williams}, O.~R. and {Zacchei}, A. and {Altieri}, B. and {Escudero Sanz}, I. and {Kohley}, R. and {Oosterbroek}, T. and {Astier}, P. and {Bacon}, D. and {Bardelli}, S. and {Baugh}, C. and {Bellagamba}, F. and {Benoist}, C. and {Bianchi}, D. and {Biviano}, A. and {Branchini}, E. and {Carbone}, C. and {Cardone}, V. and {Clements}, D. and {Colombi}, S. and {Conselice}, C. and {Cresci}, G. and {Deacon}, N. and {Dunlop}, J. and {Fedeli}, C. and {Fontanot}, F. and {Franzetti}, P. and {Giocoli}, C. and {Garcia-Bellido}, J. and {Gow}, J. and {Heavens}, A. and {Hewett}, P. and {Heymans}, C. and {Holland}, A. and {Huang}, Z. and {Ilbert}, O. and {Joachimi}, B. and {Jennins}, E. and {Kerins}, E. and {Kiessling}, A. and {Kirk}, D. and {Kotak}, R. and {Krause}, O. and {Lahav}, O. and {van Leeuwen}, F. and {Lesgourgues}, J. and {Lombardi}, M. and {Magliocchetti}, M. and {Maguire}, K. and {Majerotto}, E. and {Maoli}, R. and {Marulli}, F. and {Maurogordato}, S. and {McCracken}, H. and {McLure}, R. and {Melchiorri}, A. and {Merson}, A. and {Moresco}, M. and {Nonino}, M. and {Norberg}, P. and {Peacock}, J. and {Pello}, R. and {Penny}, M. and {Pettorino}, V. and {Di Porto}, C. and {Pozzetti}, L. and {Quercellini}, C. and {Radovich}, M. and {Rassat}, A. and {Roche}, N. and {Ronayette}, S. and {Rossetti}, E. and {Sartoris}, B. and {Schneider}, P. and {Semboloni}, E. and {Serjeant}, S. and {Simpson}, F. and {Skordis}, C. and {Smadja}, G. and {Smartt}, S. and {Spano}, P. and {Spiro}, S. and {Sullivan}, M. and {Tilquin}, A. and {Trotta}, R. and {Verde}, L. and {Wang}, Y. and {Williger}, G. and {Zhao}, G. and {Zoubian}, J. and {Zucca}, E.},
        title = "{Euclid Definition Study Report}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - Galaxy Astrophysics},
         year = 2011,
        month = oct,
          eid = {arXiv:1110.3193},
        pages = {arXiv:1110.3193},
archivePrefix = {arXiv},
       eprint = {1110.3193},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011arXiv1110.3193L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Mehta2018,
       author = {{Mehta}, Vihang and {Scarlata}, Claudia and {Capak}, Peter and {Davidzon}, Iary and {Faisst}, Andreas and {Hsieh}, Bau Ching and {Ilbert}, Olivier and {Jarvis}, Matt and {Laigle}, Clotilde and {Phillips}, John and {Silverman}, John and {Strauss}, Michael A. and {Tanaka}, Masayuki and {Bowler}, Rebecca and {Coupon}, Jean and {Foucaud}, S{\'e}bastien and {Hemmati}, Shoubaneh and {Masters}, Daniel and {McCracken}, Henry Joy and {Mobasher}, Bahram and {Ouchi}, Masami and {Shibuya}, Takatoshi and {Wang}, Wei-Hao},
        title = "{SPLASH-SXDF Multi-wavelength Photometric Catalog}",
      journal = {\apjs},
     keywords = {catalogs, galaxies: high-redshift, galaxies: photometry, methods: observational, techniques: photometric, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = apr,
       volume = {235},
       number = {2},
          eid = {36},
        pages = {36},
          doi = {10.3847/1538-4365/aab60c},
archivePrefix = {arXiv},
       eprint = {1711.05280},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ApJS..235...36M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2010ApJ...720L.131R,
       author = {{Riechers}, Dominik A. and {Capak}, Peter L. and {Carilli}, Christopher L. and {Cox}, Pierre and {Neri}, Roberto and {Scoville}, Nicholas Z. and {Schinnerer}, Eva and {Bertoldi}, Frank and {Yan}, Lin},
        title = "{A Massive Molecular Gas Reservoir in the z = 5.3 Submillimeter Galaxy AzTEC-3}",
      journal = {\apjl},
     keywords = {cosmology: observations, galaxies: active, galaxies: formation, galaxies: high-redshift, galaxies: starburst, radio lines: galaxies, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2010,
        month = sep,
       volume = {720},
       number = {2},
        pages = {L131-L136},
          doi = {10.1088/2041-8205/720/2/L131},
archivePrefix = {arXiv},
       eprint = {1008.0389},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010ApJ...720L.131R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2018ApJ...861...43P,
       author = {{Pavesi}, Riccardo and {Riechers}, Dominik A. and {Sharon}, Chelsea E. and {Smol{\v{c}}i{\'c}}, Vernesa and {Faisst}, Andreas L. and {Schinnerer}, Eva and {Carilli}, Christopher L. and {Capak}, Peter L. and {Scoville}, Nick and {Stacey}, Gordon J.},
        title = "{Hidden in Plain Sight: A Massive, Dusty Starburst in a Galaxy Protocluster at z = 5.7 in the COSMOS Field}",
      journal = {\apj},
     keywords = {cosmology: observations, galaxies: formation, galaxies: high-redshift, galaxies: ISM, galaxies: starburst, radio lines: galaxies, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2018,
        month = jul,
       volume = {861},
       number = {1},
          eid = {43},
        pages = {43},
          doi = {10.3847/1538-4357/aac6b6},
archivePrefix = {arXiv},
       eprint = {1803.08048},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ApJ...861...43P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2014ApJ...796...84R,
       author = {{Riechers}, Dominik A. and {Carilli}, Christopher L. and {Capak}, Peter L. and {Scoville}, Nicholas Z. and {Smol{\v{c}}i{\'c}}, Vernesa and {Schinnerer}, Eva and {Yun}, Min and {Cox}, Pierre and {Bertoldi}, Frank and {Karim}, Alexander and {Yan}, Lin},
        title = "{ALMA Imaging of Gas and Dust in a Galaxy Protocluster at Redshift 5.3: [C II] Emission in ``Typical'' Galaxies and Dusty Starbursts {\ensuremath{\approx}}1 Billion Years after the Big Bang}",
      journal = {\apj},
     keywords = {cosmology: observations, galaxies: active, galaxies: formation, galaxies: high-redshift, galaxies: starburst, radio lines: galaxies, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2014,
        month = dec,
       volume = {796},
       number = {2},
          eid = {84},
        pages = {84},
          doi = {10.1088/0004-637X/796/2/84},
archivePrefix = {arXiv},
       eprint = {1404.7159},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014ApJ...796...84R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2020ApJ...895...81R,
       author = {{Riechers}, Dominik A. and {Hodge}, Jacqueline A. and {Pavesi}, Riccardo and {Daddi}, Emanuele and {Decarli}, Roberto and {Ivison}, Rob J. and {Sharon}, Chelsea E. and {Smail}, Ian and {Walter}, Fabian and {Aravena}, Manuel and {Capak}, Peter L. and {Carilli}, Christopher L. and {Cox}, Pierre and {Cunha}, Elisabete da and {Dannerbauer}, Helmut and {Dickinson}, Mark and {Neri}, Roberto and {Wagg}, Jeff},
        title = "{COLDz: A High Space Density of Massive Dusty Starburst Galaxies {\ensuremath{\sim}}1 Billion Years after the Big Bang}",
      journal = {\apj},
     keywords = {Active galaxies, Galaxy evolution, Starburst galaxies, High-redshift galaxies, Infrared excess galaxies, Observational cosmology, Interstellar line emission, Submillimeter astronomy, Millimeter astronomy, 17, 594, 1570, 734, 789, 1146, 844, 1647, 1061, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = jun,
       volume = {895},
       number = {2},
          eid = {81},
        pages = {81},
          doi = {10.3847/1538-4357/ab8c48},
archivePrefix = {arXiv},
       eprint = {2004.10204},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...895...81R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2006ApJ...644..100P,
       author = {{Prescott}, M.~K.~M. and {Impey}, C.~D. and {Cool}, R.~J. and {Scoville}, N.~Z.},
        title = "{Quasars in the COSMOS Field}",
      journal = {\apj},
     keywords = {Galaxies: Quasars: Emission Lines, Galaxies: Quasars: General, Surveys, Astrophysics},
         year = 2006,
        month = jun,
       volume = {644},
       number = {1},
        pages = {100-115},
          doi = {10.1086/503325},
archivePrefix = {arXiv},
       eprint = {astro-ph/0602315},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2006ApJ...644..100P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2016A&A...595A..13H,
       author = {{Heintz}, K.~E. and {Fynbo}, J.~P.~U. and {M{\o}ller}, P. and {Milvang-Jensen}, B. and {Zabl}, J. and {Maddox}, N. and {Krogager}, J. -K. and {Geier}, S. and {Vestergaard}, M. and {Noterdaeme}, P. and {Ledoux}, C.},
        title = "{Determining the fraction of reddened quasars in COSMOS with multiple selection techniques from X-ray to radio wavelengths}",
      journal = {\aap},
     keywords = {galaxies: active, quasars: general, surveys, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2016,
        month = oct,
       volume = {595},
          eid = {A13},
        pages = {A13},
          doi = {10.1051/0004-6361/201628836},
archivePrefix = {arXiv},
       eprint = {1605.00701},
 primaryClass = {astro-ph.HE},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016A&A...595A..13H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{2012SPIE.8446E..0JM,
       author = {{McLean}, Ian S. and {Steidel}, Charles C. and {Epps}, Harland W. and {Konidaris}, Nicholas and {Matthews}, Keith Y. and {Adkins}, Sean and {Aliado}, Theodore and {Brims}, George and {Canfield}, John M. and {Cromer}, John L. and {Fucik}, Jason and {Kulas}, Kristin and {Mace}, Greg and {Magnone}, Ken and {Rodriguez}, Hector and {Rudie}, Gwen and {Trainor}, Ryan and {Wang}, Eric and {Weber}, Bob and {Weiss}, Jason},
        title = "{MOSFIRE, the multi-object spectrometer for infra-red exploration at the Keck Observatory}",
    booktitle = {Ground-based and Airborne Instrumentation for Astronomy IV},
         year = 2012,
       editor = {{McLean}, Ian S. and {Ramsay}, Suzanne K. and {Takami}, Hideki},
       series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
       volume = {8446},
        month = sep,
          eid = {84460J},
        pages = {84460J},
          doi = {10.1117/12.924794},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012SPIE.8446E..0JM},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2003AJ....125.1107L,
       author = {{Labb{\'e}}, Ivo and {Franx}, Marijn and {Rudnick}, Gregory and {F{\"o}rster Schreiber}, Natascha M. and {Rix}, Hans-Walter and {Moorwood}, Alan and {van Dokkum}, Pieter G. and {van der Werf}, Paul and {R{\"o}ttgering}, Huub and {van Starkenburg}, Lottie and {van der Wel}, Arjen and {Kuijken}, Konrad and {Daddi}, Emanuele},
        title = "{Ultradeep Near-Infrared ISAAC Observations of the Hubble Deep Field South: Observations, Reduction, Multicolor Catalog, and Photometric Redshifts}",
      journal = {\aj},
     keywords = {Galaxies: Evolution, Galaxies: High-Redshift, Galaxies: Photometry, Astrophysics},
         year = 2003,
        month = mar,
       volume = {125},
       number = {3},
        pages = {1107-1123},
          doi = {10.1086/346140},
archivePrefix = {arXiv},
       eprint = {astro-ph/0212236},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2003AJ....125.1107L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2013A&A...558A..33A,
       author = {{Astropy Collaboration} and {Robitaille}, Thomas P. and {Tollerud}, Erik J. and {Greenfield}, Perry and {Droettboom}, Michael and {Bray}, Erik and {Aldcroft}, Tom and {Davis}, Matt and {Ginsburg}, Adam and {Price-Whelan}, Adrian M. and {Kerzendorf}, Wolfgang E. and {Conley}, Alexander and {Crighton}, Neil and {Barbary}, Kyle and {Muna}, Demitri and {Ferguson}, Henry and {Grollier}, Fr{\'e}d{\'e}ric and {Parikh}, Madhura M. and {Nair}, Prasanth H. and {Unther}, Hans M. and {Deil}, Christoph and {Woillez}, Julien and {Conseil}, Simon and {Kramer}, Roban and {Turner}, James E.~H. and {Singer}, Leo and {Fox}, Ryan and {Weaver}, Benjamin A. and {Zabalza}, Victor and {Edwards}, Zachary I. and {Azalee Bostroem}, K. and {Burke}, D.~J. and {Casey}, Andrew R. and {Crawford}, Steven M. and {Dencheva}, Nadia and {Ely}, Justin and {Jenness}, Tim and {Labrie}, Kathleen and {Lim}, Pey Lian and {Pierfederici}, Francesco and {Pontzen}, Andrew and {Ptak}, Andy and {Refsdal}, Brian and {Servillat}, Mathieu and {Streicher}, Ole},
        title = "{Astropy: A community Python package for astronomy}",
      journal = {\aap},
     keywords = {methods: data analysis, methods: miscellaneous, virtual observatory tools, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2013,
        month = oct,
       volume = {558},
          eid = {A33},
        pages = {A33},
          doi = {10.1051/0004-6361/201322068},
archivePrefix = {arXiv},
       eprint = {1307.6212},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013A&A...558A..33A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{numpy2011,
  author={S. {van der Walt} and S. C. {Colbert} and G. {Varoquaux}},
  journal={Computing in Science   Engineering}, 
  title={The NumPy Array: A Structure for Efficient Numerical Computation}, 
  year={2011},
  volume={13},
  number={2},
  pages={22-30},
  doi={10.1109/MCSE.2011.37}}

@ARTICLE{matplotlib2007,
  author={J. D. {Hunter}},
  journal={Computing in Science   Engineering}, 
  title={Matplotlib: A 2D Graphics Environment}, 
  year={2007},
  volume={9},
  number={3},
  pages={90-95},
  doi={10.1109/MCSE.2007.55}}
  

@ARTICLE{Scoville2007b,
       author = {{Scoville}, N. and {Abraham}, R.~G. and {Aussel}, H. and {Barnes}, J.~E. and {Benson}, A. and {Blain}, A.~W. and {Calzetti}, D. and {Comastri}, A. and {Capak}, P. and {Carilli}, C. and {Carlstrom}, J.~E. and {Carollo}, C.~M. and {Colbert}, J. and {Daddi}, E. and {Ellis}, R.~S. and {Elvis}, M. and {Ewald}, S.~P. and {Fall}, M. and {Franceschini}, A. and {Giavalisco}, M. and {Green}, W. and {Griffiths}, R.~E. and {Guzzo}, L. and {Hasinger}, G. and {Impey}, C. and {Kneib}, J. -P. and {Koda}, J. and {Koekemoer}, A. and {Lefevre}, O. and {Lilly}, S. and {Liu}, C.~T. and {McCracken}, H.~J. and {Massey}, R. and {Mellier}, Y. and {Miyazaki}, S. and {Mobasher}, B. and {Mould}, J. and {Norman}, C. and {Refregier}, A. and {Renzini}, A. and {Rhodes}, J. and {Rich}, M. and {Sanders}, D.~B. and {Schiminovich}, D. and {Schinnerer}, E. and {Scodeggio}, M. and {Sheth}, K. and {Shopbell}, P.~L. and {Taniguchi}, Y. and {Tyson}, N.~D. and {Urry}, C.~M. and {Van Waerbeke}, L. and {Vettolani}, P. and {White}, S.~D.~M. and {Yan}, L.},
        title = "{COSMOS: Hubble Space Telescope Observations}",
      journal = {\apjs},
     keywords = {Cosmology: Observations, Cosmology: Dark Matter, Galaxies: Evolution, Galaxies: Formation, Cosmology: Large-Scale Structure of Universe, Surveys, Astrophysics},
         year = 2007,
        month = sep,
       volume = {172},
       number = {1},
        pages = {38-45},
          doi = {10.1086/516580},
archivePrefix = {arXiv},
       eprint = {astro-ph/0612306},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007ApJS..172...38S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Stefanon2019,
       author = {{Stefanon}, Mauro and {Labb{\'e}}, Ivo and {Bouwens}, Rychard J. and {Oesch}, Pascal and {Ashby}, Matthew L.~N. and {Caputi}, Karina I. and {Franx}, Marijn and {Fynbo}, Johan P.~U. and {Illingworth}, Garth D. and {Le F{\`e}vre}, Olivier and {Marchesini}, Danilo and {McCracken}, Henry J. and {Milvang-Jensen}, Bo and {Muzzin}, Adam and {van Dokkum}, Pieter},
        title = "{The Brightest z {\ensuremath{\gtrsim}} 8 Galaxies over the COSMOS UltraVISTA Field}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, galaxies: luminosity function, mass function, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = sep,
       volume = {883},
       number = {1},
          eid = {99},
        pages = {99},
          doi = {10.3847/1538-4357/ab3792},
archivePrefix = {arXiv},
       eprint = {1902.10713},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...883...99S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{FS_HDF_1999,
       author = {{Fern{\'a}ndez-Soto}, Alberto and {Lanzetta}, Kenneth M. and {Yahil}, Amos},
        title = "{A New Catalog of Photometric Redshifts in the Hubble Deep Field}",
      journal = {\apj},
     keywords = {COSMOLOGY: OBSERVATIONS, GALAXIES: DISTANCES AND REDSHIFTS, GALAXIES: PHOTOMETRY, GALAXIES: STATISTICS, Cosmology: Observations, Galaxies: Distances and Redshifts, Galaxies: Photometry, Galaxies: Statistics, Astrophysics},
         year = 1999,
        month = mar,
       volume = {513},
       number = {1},
        pages = {34-50},
          doi = {10.1086/306847},
archivePrefix = {arXiv},
       eprint = {astro-ph/9809126},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1999ApJ...513...34F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Labbe_2006,
       author = {{Labb{\'e}}, Ivo and {Bouwens}, Rychard and {Illingworth}, G.~D. and {Franx}, M.},
        title = "{Spitzer IRAC Confirmation of z$_{850}$-Dropout Galaxies in the Hubble Ultra Deep Field: Stellar Masses and Ages at z \raisebox{-0.5ex}\textasciitilde 7}",
      journal = {\apjl},
     keywords = {Galaxies: Evolution, Galaxies: High-Redshift, Infrared: Galaxies, Astrophysics},
         year = 2006,
        month = oct,
       volume = {649},
       number = {2},
        pages = {L67-L70},
          doi = {10.1086/508512},
archivePrefix = {arXiv},
       eprint = {astro-ph/0608444},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2006ApJ...649L..67L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Labbe_2015,
       author = {{Labb{\'e}}, I. and {Oesch}, P.~A. and {Illingworth}, G.~D. and {van Dokkum}, P.~G. and {Bouwens}, R.~J. and {Franx}, M. and {Carollo}, C.~M. and {Trenti}, M. and {Holden}, B. and {Smit}, R. and {Gonz{\'a}lez}, V. and {Magee}, D. and {Stiavelli}, M. and {Stefanon}, M.},
        title = "{Ultradeep IRAC Imaging Over the HUDF and GOODS-South: Survey Design and Imaging Data Release}",
      journal = {\apjs},
     keywords = {galaxies: high-redshift, surveys, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2015,
        month = dec,
       volume = {221},
       number = {2},
          eid = {23},
        pages = {23},
          doi = {10.1088/0067-0049/221/2/23},
archivePrefix = {arXiv},
       eprint = {1507.08313},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015ApJS..221...23L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Salvato2011,
       author = {{Salvato}, M. and {Ilbert}, O. and {Hasinger}, G. and {Rau}, A. and {Civano}, F. and {Zamorani}, G. and {Brusa}, M. and {Elvis}, M. and {Vignali}, C. and {Aussel}, H. and {Comastri}, A. and {Fiore}, F. and {Le Floc'h}, E. and {Mainieri}, V. and {Bardelli}, S. and {Bolzonella}, M. and {Bongiorno}, A. and {Capak}, P. and {Caputi}, K. and {Cappelluti}, N. and {Carollo}, C.~M. and {Contini}, T. and {Garilli}, B. and {Iovino}, A. and {Fotopoulou}, S. and {Fruscione}, A. and {Gilli}, R. and {Halliday}, C. and {Kneib}, J. -P. and {Kakazu}, Y. and {Kartaltepe}, J.~S. and {Koekemoer}, A.~M. and {Kovac}, K. and {Ideue}, Y. and {Ikeda}, H. and {Impey}, C.~D. and {Le Fevre}, O. and {Lamareille}, F. and {Lanzuisi}, G. and {Le Borgne}, J. -F. and {Le Brun}, V. and {Lilly}, S. and {Maier}, C. and {Manohar}, S. and {Masters}, D. and {McCracken}, H. and {Messias}, H. and {Mignoli}, M. and {Mobasher}, B. and {Nagao}, T. and {Pello}, R. and {Puccetti}, S. and {Perez-Montero}, E. and {Renzini}, A. and {Sargent}, M. and {Sanders}, D.~B. and {Scodeggio}, M. and {Scoville}, N. and {Shopbell}, P. and {Silvermann}, J. and {Taniguchi}, Y. and {Tasca}, L. and {Tresse}, L. and {Trump}, J.~R. and {Zucca}, E.},
        title = "{Dissecting Photometric Redshift for Active Galactic Nucleus Using XMM- and Chandra-COSMOS Samples}",
      journal = {\apj},
     keywords = {galaxies: active, galaxies: distances and redshifts, methods: data analysis, surveys, techniques: photometric, X-rays: galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2011,
        month = dec,
       volume = {742},
       number = {2},
          eid = {61},
        pages = {61},
          doi = {10.1088/0004-637X/742/2/61},
archivePrefix = {arXiv},
       eprint = {1108.6061},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJ...742...61S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Salvato2009ApJ,
       author = {{Salvato}, M. and {Hasinger}, G. and {Ilbert}, O. and {Zamorani}, G. and {Brusa}, M. and {Scoville}, N.~Z. and {Rau}, A. and {Capak}, P. and {Arnouts}, S. and {Aussel}, H. and {Bolzonella}, M. and {Buongiorno}, A. and {Cappelluti}, N. and {Caputi}, K. and {Civano}, F. and {Cook}, R. and {Elvis}, M. and {Gilli}, R. and {Jahnke}, K. and {Kartaltepe}, J.~S. and {Impey}, C.~D. and {Lamareille}, F. and {Le Floc'h}, E. and {Lilly}, S. and {Mainieri}, V. and {McCarthy}, P. and {McCracken}, H. and {Mignoli}, M. and {Mobasher}, B. and {Murayama}, T. and {Sasaki}, S. and {Sanders}, D.~B. and {Schiminovich}, D. and {Shioya}, Y. and {Shopbell}, P. and {Silverman}, J. and {Smol{\v{c}}i{\'c}}, V. and {Surace}, J. and {Taniguchi}, Y. and {Thompson}, D. and {Trump}, J.~R. and {Urry}, M. and {Zamojski}, M.},
        title = "{Photometric Redshift and Classification for the XMM-COSMOS Sources}",
      journal = {\apj},
     keywords = {catalogs, galaxies: active, methods: miscellaneous, Astrophysics},
         year = 2009,
        month = jan,
       volume = {690},
       number = {2},
        pages = {1250-1263},
          doi = {10.1088/0004-637X/690/2/1250},
archivePrefix = {arXiv},
       eprint = {0809.2098},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009ApJ...690.1250S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Teplitz_2013,
       author = {{Teplitz}, Harry I. and {Rafelski}, Marc and {Kurczynski}, Peter and {Bond}, Nicholas A. and {Grogin}, Norman and {Koekemoer}, Anton M. and {Atek}, Hakim and {Brown}, Thomas M. and {Coe}, Dan and {Colbert}, James W. and {Ferguson}, Henry C. and {Finkelstein}, Steven L. and {Gardner}, Jonathan P. and {Gawiser}, Eric and {Giavalisco}, Mauro and {Gronwall}, Caryl and {Hanish}, Daniel J. and {Lee}, Kyoung-Soo and {de Mello}, Duilia F. and {Ravindranath}, Swara and {Ryan}, Russell E. and {Siana}, Brian D. and {Scarlata}, Claudia and {Soto}, Emmaris and {Voyer}, Elysse N. and {Wolfe}, Arthur M.},
        title = "{UVUDF: Ultraviolet Imaging of the Hubble Ultra Deep Field with Wide-Field Camera 3}",
      journal = {\aj},
     keywords = {cosmology: observations, galaxies: evolution, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = dec,
       volume = {146},
       number = {6},
          eid = {159},
        pages = {159},
          doi = {10.1088/0004-6256/146/6/159},
archivePrefix = {arXiv},
       eprint = {1305.1357},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013AJ....146..159T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Ellis_2013,
       author = {{Ellis}, Richard S. and {McLure}, Ross J. and {Dunlop}, James S. and {Robertson}, Brant E. and {Ono}, Yoshiaki and {Schenker}, Matthew A. and {Koekemoer}, Anton and {Bowler}, Rebecca A.~A. and {Ouchi}, Masami and {Rogers}, Alexander B. and {Curtis-Lake}, Emma and {Schneider}, Evan and {Charlot}, Stephane and {Stark}, Daniel P. and {Furlanetto}, Steven R. and {Cirasuolo}, Michele},
        title = "{The Abundance of Star-forming Galaxies in the Redshift Range 8.5-12: New Results from the 2012 Hubble Ultra Deep Field Campaign}",
      journal = {\apjl},
     keywords = {dark ages, reionization, first stars, galaxies: evolution, galaxies: formation, galaxies: stellar content, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = jan,
       volume = {763},
       number = {1},
          eid = {L7},
        pages = {L7},
          doi = {10.1088/2041-8205/763/1/L7},
archivePrefix = {arXiv},
       eprint = {1211.6804},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJ...763L...7E},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Allard_2012,
       author = {{Allard}, F. and {Homeier}, D. and {Freytag}, B.},
        title = "{Models of very-low-mass stars, brown dwarfs and exoplanets}",
      journal = {Philosophical Transactions of the Royal Society of London Series A},
     keywords = {Astrophysics - Solar and Stellar Astrophysics},
         year = 2012,
        month = jun,
       volume = {370},
       number = {1968},
        pages = {2765-2777},
          doi = {10.1098/rsta.2011.0269},
archivePrefix = {arXiv},
       eprint = {1112.3591},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012RSPTA.370.2765A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Mobasher_1996,
       author = {{Mobasher}, B. and {Rowan-Robinson}, M. and {Georgakakis}, A. and {Eaton}, N.},
        title = "{The nature of the faint galaxies in the Hubble Deep Field}",
      journal = {\mnras},
     keywords = {GALAXIES: EVOLUTION, GALAXIES: LUMINOSITY FUNCTION, MASS FUNCTION, COSMOLOGY: OBSERVATIONS, Astrophysics},
         year = 1996,
        month = sep,
       volume = {282},
       number = {1},
        pages = {L7-L13},
          doi = {10.1093/mnras/282.1.L7},
archivePrefix = {arXiv},
       eprint = {astro-ph/9604118},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1996MNRAS.282L...7M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Sawicki_1997,
       author = {{Sawicki}, M.~J. and {Lin}, H. and {Yee}, H.~K.~C.},
        title = "{Evolution of the Galaxy Population Based on Photometric Redshifts in the Hubble Deep Field}",
      journal = {\aj},
     keywords = {Astrophysics},
         year = 1997,
        month = jan,
       volume = {113},
        pages = {1-12},
          doi = {10.1086/118231},
archivePrefix = {arXiv},
       eprint = {astro-ph/9610100},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1997AJ....113....1S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Trenti_2008,
       author = {{Trenti}, M. and {Stiavelli}, M.},
        title = "{Cosmic Variance and Its Effect on the Luminosity Function Determination in Deep High-z Surveys}",
      journal = {\apj},
     keywords = {galaxies: high-redshift, galaxies: statistics, large-scale structure of universe, Astrophysics},
         year = 2008,
        month = apr,
       volume = {676},
       number = {2},
        pages = {767-780},
          doi = {10.1086/528674},
archivePrefix = {arXiv},
       eprint = {0712.0398},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2008ApJ...676..767T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2018AJ....156..123A,
       author = {{Astropy Collaboration} and {Price-Whelan}, A.~M. and {Sip{\H{o}}cz}, B.~M. and {G{\"u}nther}, H.~M. and {Lim}, P.~L. and {Crawford}, S.~M. and {Conseil}, S. and {Shupe}, D.~L. and {Craig}, M.~W. and {Dencheva}, N. and {Ginsburg}, A. and {VanderPlas}, J.~T. and {Bradley}, L.~D. and {P{\'e}rez-Su{\'a}rez}, D. and {de Val-Borro}, M. and {Aldcroft}, T.~L. and {Cruz}, K.~L. and {Robitaille}, T.~P. and {Tollerud}, E.~J. and {Ardelean}, C. and {Babej}, T. and {Bach}, Y.~P. and {Bachetti}, M. and {Bakanov}, A.~V. and {Bamford}, S.~P. and {Barentsen}, G. and {Barmby}, P. and {Baumbach}, A. and {Berry}, K.~L. and {Biscani}, F. and {Boquien}, M. and {Bostroem}, K.~A. and {Bouma}, L.~G. and {Brammer}, G.~B. and {Bray}, E.~M. and {Breytenbach}, H. and {Buddelmeijer}, H. and {Burke}, D.~J. and {Calderone}, G. and {Cano Rodr{\'\i}guez}, J.~L. and {Cara}, M. and {Cardoso}, J.~V.~M. and {Cheedella}, S. and {Copin}, Y. and {Corrales}, L. and {Crichton}, D. and {D'Avella}, D. and {Deil}, C. and {Depagne}, {\'E}. and {Dietrich}, J.~P. and {Donath}, A. and {Droettboom}, M. and {Earl}, N. and {Erben}, T. and {Fabbro}, S. and {Ferreira}, L.~A. and {Finethy}, T. and {Fox}, R.~T. and {Garrison}, L.~H. and {Gibbons}, S.~L.~J. and {Goldstein}, D.~A. and {Gommers}, R. and {Greco}, J.~P. and {Greenfield}, P. and {Groener}, A.~M. and {Grollier}, F. and {Hagen}, A. and {Hirst}, P. and {Homeier}, D. and {Horton}, A.~J. and {Hosseinzadeh}, G. and {Hu}, L. and {Hunkeler}, J.~S. and {Ivezi{\'c}}, {\v{Z}}. and {Jain}, A. and {Jenness}, T. and {Kanarek}, G. and {Kendrew}, S. and {Kern}, N.~S. and {Kerzendorf}, W.~E. and {Khvalko}, A. and {King}, J. and {Kirkby}, D. and {Kulkarni}, A.~M. and {Kumar}, A. and {Lee}, A. and {Lenz}, D. and {Littlefair}, S.~P. and {Ma}, Z. and {Macleod}, D.~M. and {Mastropietro}, M. and {McCully}, C. and {Montagnac}, S. and {Morris}, B.~M. and {Mueller}, M. and {Mumford}, S.~J. and {Muna}, D. and {Murphy}, N.~A. and {Nelson}, S. and {Nguyen}, G.~H. and {Ninan}, J.~P. and {N{\"o}the}, M. and {Ogaz}, S. and {Oh}, S. and {Parejko}, J.~K. and {Parley}, N. and {Pascual}, S. and {Patil}, R. and {Patil}, A.~A. and {Plunkett}, A.~L. and {Prochaska}, J.~X. and {Rastogi}, T. and {Reddy Janga}, V. and {Sabater}, J. and {Sakurikar}, P. and {Seifert}, M. and {Sherbert}, L.~E. and {Sherwood-Taylor}, H. and {Shih}, A.~Y. and {Sick}, J. and {Silbiger}, M.~T. and {Singanamalla}, S. and {Singer}, L.~P. and {Sladen}, P.~H. and {Sooley}, K.~A. and {Sornarajah}, S. and {Streicher}, O. and {Teuben}, P. and {Thomas}, S.~W. and {Tremblay}, G.~R. and {Turner}, J.~E.~H. and {Terr{\'o}n}, V. and {van Kerkwijk}, M.~H. and {de la Vega}, A. and {Watkins}, L.~L. and {Weaver}, B.~A. and {Whitmore}, J.~B. and {Woillez}, J. and {Zabalza}, V. and {Astropy Contributors}},
        title = "{The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package}",
      journal = {\aj},
     keywords = {methods: data analysis, methods: miscellaneous, methods: statistical, reference systems, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2018,
        month = sep,
       volume = {156},
       number = {3},
          eid = {123},
        pages = {123},
          doi = {10.3847/1538-3881/aabc4f},
archivePrefix = {arXiv},
       eprint = {1801.02634},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018AJ....156..123A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{2016ascl.soft04008L,
       author = {{Lang}, Dustin and {Hogg}, David W. and {Mykytyn}, David},
        title = "{The Tractor: Probabilistic astronomical source detection and measurement}",
     keywords = {Software},
         year = 2016,
        month = apr,
          eid = {ascl:1604.008},
        pages = {ascl:1604.008},
archivePrefix = {ascl},
       eprint = {1604.008},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016ascl.soft04008L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{2019amgp.confE...9W,
       author = {{Weaver}, John and {Toft}, Sune and {Davidzon}, Iary and {Capak}, Peter and {McCracken}, Henry},
        title = "{The Farmer: Improved model-based photometry for the next generation of galaxy surveys}",
     keywords = {Galaxy Evolution, Astrostatistics, Galaxies, Software, Zenodo community app-iasfmi-2019},
    booktitle = {The Art of Measuring Galaxy Physical Properties},
         year = 2019,
        month = nov,
          eid = {9},
        pages = {9},
          doi = {10.5281/zenodo.3554205},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019amgp.confE...9W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{arcilaosejo2013,
       author = {{Arcila-Osejo}, Liz and {Sawicki}, Marcin},
        title = "{The numbers of z {\textasciitilde} 2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: luminosity function, mass function, Astrophysics - Galaxy Astrophysics, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2013,
        month = oct,
       volume = {435},
       number = {1},
        pages = {845-860},
          doi = {10.1093/mnras/stt1354},
archivePrefix = {arXiv},
       eprint = {1307.6094},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013MNRAS.435..845A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{sawicki1998,
       author = {{Sawicki}, Marcin and {Yee}, H.~K.~C.},
        title = "{Optical-Infrared Spectral Energy Distributions of Z > 2 Lyman Break Galaxies}",
      journal = {\aj},
     keywords = {COSMOLOGY: OBSERVATIONS, EARLY UNIVERSE, GALAXIES: STARBURST, Astrophysics},
         year = 1998,
        month = apr,
       volume = {115},
       number = {4},
        pages = {1329-1339},
          doi = {10.1086/300291},
archivePrefix = {arXiv},
       eprint = {astro-ph/9712216},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1998AJ....115.1329S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{Moneti2019,
       author = {{Moneti}, A. and {McCracken}, H. J. and {Rouberol}, S. and {Herent}, O. and {Mellier}, Y. and {Dunlop}, J. and {Le F{\'e}vre}, O. and {Franx}, M. and {Fynbo}, J. and {Bowler}, R. and {Caputi}, K. and {Kauffmann}, O. and {Milvang-Jensen}, B. and {Gonzalez-Fernandez}, C. and {Gonzalez-Solares}, M. and {Irwin}, M. and {Lewis}, J. and {Blake}, R. and {Cross}, N. and {Read}, M. and {Sutorius}, E.},
        title = "{The Fourth UltraVISTA data release}",
     keywords = {Data products},
         year = 2019,
        month = mar,
howpublished = {ESO},
}

@MISC{Kriek2018,
       author = {{Kriek}, Mariska and {van Dokkum}, Pieter G. and {Labb{\'e}}, Ivo and {Franx}, Marijn and {Illingworth}, Garth D. and {Marchesini}, Danilo and {Quadri}, Ryan F. and {Aird}, James and {Coil}, Alison L. and {Georgakakis}, Antonis},
        title = "{FAST: Fitting and Assessment of Synthetic Templates}",
     keywords = {Software},
         year = 2018,
        month = mar,
          eid = {ascl:1803.008},
        pages = {ascl:1803.008},
archivePrefix = {ascl},
       eprint = {1803.008},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ascl.soft03008K},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Sorba2018,
       author = {{Sorba}, Robert and {Sawicki}, Marcin},
        title = "{Spatially unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem}",
      journal = {\mnras},
     keywords = {galaxies: high-redshift, galaxies: luminosity function, mass function, galaxies: statistics, galaxies: stellar content, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = may,
       volume = {476},
       number = {2},
        pages = {1532-1547},
          doi = {10.1093/mnras/sty186},
archivePrefix = {arXiv},
       eprint = {1801.07368},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.476.1532S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Leja2019,
       author = {{Leja}, Joel and {Johnson}, Benjamin D. and {Conroy}, Charlie and {van Dokkum}, Pieter and {Speagle}, Joshua S. and {Brammer}, Gabriel and {Momcheva}, Ivelina and {Skelton}, Rosalind and {Whitaker}, Katherine E. and {Franx}, Marijn and {Nelson}, Erica J.},
        title = "{An Older, More Quiescent Universe from Panchromatic SED Fitting of the 3D-HST Survey}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: fundamental parameters, galaxies: star formation, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = jun,
       volume = {877},
       number = {2},
          eid = {140},
        pages = {140},
          doi = {10.3847/1538-4357/ab1d5a},
archivePrefix = {arXiv},
       eprint = {1812.05608},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...877..140L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Abdurrouf2018,
       author = {{Abdurro'uf} and {Akiyama}, Masayuki},
        title = "{Evolution of spatially resolved star formation main sequence and surface density profiles in massive disc galaxies at 0 {\ensuremath{\lesssim}} z {\ensuremath{\lesssim}} 1: inside-out stellar mass buildup and quenching}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: fundamental parameters, galaxies: spiral, galaxies: star formation, galaxies: structure, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = oct,
       volume = {479},
       number = {4},
        pages = {5083-5100},
          doi = {10.1093/mnras/sty1771},
archivePrefix = {arXiv},
       eprint = {1802.03782},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.479.5083A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Mosleh2020,
       author = {{Mosleh}, Moein and {Hosseinnejad}, Shiva and {Hosseini-ShahiSavandi}, S. Zahra and {Tacchella}, Sandro},
        title = "{Galaxy Sizes Since z = 2 from the Perspective of Stellar Mass Distribution within Galaxies}",
      journal = {\apj},
     keywords = {Galaxy structure, Galaxy evolution, Galaxy mass distribution, Galaxy radii, 622, 594, 606, 617, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = dec,
       volume = {905},
       number = {2},
          eid = {170},
        pages = {170},
          doi = {10.3847/1538-4357/abc7cc},
archivePrefix = {arXiv},
       eprint = {2011.04656},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...905..170M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Croton2013,
       author = {{Croton}, Darren J.},
        title = "{Damn You, Little h! (Or, Real-World Applications of the Hubble Constant Using Observed and Simulated Data)}",
      journal = {\pasa},
     keywords = {cosmology, galaxies, methods: observational, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2013,
        month = oct,
       volume = {30},
          eid = {e052},
        pages = {e052},
          doi = {10.1017/pasa.2013.31},
archivePrefix = {arXiv},
       eprint = {1308.4150},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013PASA...30...52C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{Weaver2021_jwst,
       author = {{Weaver}, John Raymond and {Brammer}, Gabriel and {Casey}, Caitlin M. and {Chartab Soltani}, Nima and {Davidzon}, Iary and {Faisst}, Andreas L. and {Finkelstein}, Steven L. and {Fujimoto}, Seiji and {Gould}, Katriona Mai Landau and {Ilbert}, Olivier and {Jespersen}, Christian Kragh and {Kauffmann}, Olivier Benjamin and {Magdis}, Georgios and {McCracken}, Henry Joy and {McPartland}, Conor and {Milvang-Jensen}, Bo and {Mobasher}, Bahram and {Oesch}, Pascal and {Sanders}, David B. and {Scarlata}, Claudia and {Shuntov}, Marko and {Steinhardt}, Charles Louis and {Stern}, Daniel K. and {Szapudi}, Istvan and {Toft}, Sune and {Valentino}, Francesco Maria and {Zalesky}, Lukas},
        title = "{Beasts in the Bubbles: Characterizing ultra-luminous galaxies at Cosmic Dawn}",
 howpublished = {JWST Proposal. Cycle 1},
         year = 2021,
        month = mar,
        pages = {2659},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021jwst.prop.2659W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Long2022,
       author = {{Long}, Arianna S. and {Casey}, Caitlin M. and {Lagos}, Claudia del P. and {Lambrides}, Erini L. and {Zavala}, Jorge A. and {Champagne}, Jaclyn and {Cooper}, Olivia R. and {Cooray}, Asantha R.},
        title = "{Missing Giants: Predictions on Dust-Obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = nov,
          eid = {arXiv:2211.02072},
        pages = {arXiv:2211.02072},
archivePrefix = {arXiv},
       eprint = {2211.02072},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv221102072L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Tanaka2015,
       author = {{Tanaka}, Masayuki},
        title = "{Photometric Redshift with Bayesian Priors on Physical Properties of Galaxies}",
      journal = {\apj},
     keywords = {galaxies: distances and redshifts, surveys, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2015,
        month = mar,
       volume = {801},
       number = {1},
          eid = {20},
        pages = {20},
          doi = {10.1088/0004-637X/801/1/20},
archivePrefix = {arXiv},
       eprint = {1501.02047},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015ApJ...801...20T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Casey2022,
       author = {{Casey}, Caitlin M. and {Kartaltepe}, Jeyhan S. and {Drakos}, Nicole E. and {Franco}, Maximilien and {Ilbert}, Olivier and {Rose}, Caitlin and {Cox}, Isabella G. and {Nightingale}, James W. and {Robertson}, Brant E. and {Silverman}, John D. and {Koekemoer}, Anton M. and {Massey}, Richard and {McCracken}, Henry Joy and {Rhodes}, Jason and {Akins}, Hollis B. and {Amvrosiadis}, Aristeidis and {Arango-Toro}, Rafael C. and {Bagley}, Micaela B. and {Capak}, Peter L. and {Champagne}, Jaclyn B. and {Chartab}, Nima and {Chavez Ortiz}, Oscar A. and {Cooke}, Kevin C. and {Cooper}, Olivia R. and {Darvish}, Behnam and {Ding}, Xuheng and {Faisst}, Andreas L. and {Finkelstein}, Steven L. and {Fujimoto}, Seiji and {Gentile}, Fabrizio and {Gillman}, Steven and {Gould}, Katriona M.~L. and {Gozaliasl}, Ghassem and {Harish}, Santosh and {Hayward}, Christopher C. and {He}, Qiuhan and {Hemmati}, Shoubaneh and {Hirschmann}, Michaela and {Jin}, Shuowen and {Khostovan}, Ali Ahmad and {Kokorev}, Vasily and {Lambrides}, Erini and {Laigle}, Clotilde and {Leung}, Gene C.~K. and {Liu}, Daizhong and {Liaudat}, Tobias and {Long}, Arianna S. and {Magdis}, Georgios and {Mahler}, Guillaume and {Mainieri}, Vincenzo and {Manning}, Sinclaire M. and {Maraston}, Claudia and {Martin}, Crystal L. and {McCleary}, Jacqueline E. and {McKinney}, Jed and {McPartland}, Conor J.~R. and {Mobasher}, Bahram and {Pattnaik}, Rohan and {Renzini}, Alvio and {Rich}, R. Michael and {Sanders}, David B. and {Sattari}, Zahra and {Scognamiglio}, Diana and {Scoville}, Nick and {Sheth}, Kartik and {Shuntov}, Marko and {Sparre}, Martin and {Suzuki}, Tomoko L. and {Talia}, Margherita and {Toft}, Sune and {Trakhtenbrot}, Benny and {Urry}, C. Megan and {Valentino}, Francesco and {Vanderhoof}, Brittany N. and {Vardoulaki}, Eleni and {Weaver}, John R. and {Whitaker}, Katherine E. and {Wilkins}, Stephen M. and {Yang}, Lilan and {Zavala}, Jorge A.},
        title = "{COSMOS-Web: An Overview of the JWST Cosmic Origins Survey}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2022,
        month = nov,
          eid = {arXiv:2211.07865},
        pages = {arXiv:2211.07865},
archivePrefix = {arXiv},
       eprint = {2211.07865},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv221107865C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Marchesini2022,
       author = {{Marchesini}, Danilo and {Brammer}, Gabriel and {Morishita}, Takahiro and {Bergamini}, Pietro and {Wang}, Xin and {Bradac}, Marusa and {Roberts-Borsani}, Guido and {Strait}, Victoria and {Treu}, Tommaso and {Fontana}, Adriano and {Jones}, Tucker and {Santini}, Paola and {Vulcani}, Benedetta and {Acebron}, Ana and {Calabr{\`o}}, Antonello and {Castellano}, Marco and {Glazebrook}, Karl and {Grillo}, Claudio and {Mercurio}, Amata and {Nanayakkara}, Themiya and {Rosati}, Piero and {Tubthong}, Chanita and {Vanzella}, Eros},
        title = "{Early results from GLASS-JWST. IX: First spectroscopic confirmation of low-mass quiescent galaxies at $z>2$ with NIRISS}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = jul,
          eid = {arXiv:2207.13625},
        pages = {arXiv:2207.13625},
archivePrefix = {arXiv},
       eprint = {2207.13625},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220713625M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Donnan2022,
       author = {{Donnan}, C.~T. and {McLeod}, D.~J. and {Dunlop}, J.~S. and {McLure}, R.~J. and {Carnall}, A.~C. and {Begley}, R. and {Cullen}, F. and {Hamadouche}, M.~L. and {Bowler}, R.~A.~A. and {Magee}, D. and {McCracken}, H.~J. and {Milvang-Jensen}, B. and {Moneti}, A. and {Targett}, T.},
        title = "{The evolution of the galaxy UV luminosity function at redshifts z \raisebox{-0.5ex}\textasciitilde 8-15 from deep JWST and ground-based near-infrared imaging}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = jul,
          eid = {arXiv:2207.12356},
        pages = {arXiv:2207.12356},
archivePrefix = {arXiv},
       eprint = {2207.12356},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220712356D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Weaver2022_catalog,
       author = {{Weaver}, J.~R. and {Kauffmann}, O.~B. and {Ilbert}, O. and {McCracken}, H.~J. and {Moneti}, A. and {Toft}, S. and {Brammer}, G. and {Shuntov}, M. and {Davidzon}, I. and {Hsieh}, B.~C. and {Laigle}, C. and {Anastasiou}, A. and {Jespersen}, C.~K. and {Vinther}, J. and {Capak}, P. and {Casey}, C.~M. and {McPartland}, C.~J.~R. and {Milvang-Jensen}, B. and {Mobasher}, B. and {Sanders}, D.~B. and {Zalesky}, L. and {Arnouts}, S. and {Aussel}, H. and {Dunlop}, J.~S. and {Faisst}, A. and {Franx}, M. and {Furtak}, L.~J. and {Fynbo}, J.~P.~U. and {Gould}, K.~M.~L. and {Greve}, T.~R. and {Gwyn}, S. and {Kartaltepe}, J.~S. and {Kashino}, D. and {Koekemoer}, A.~M. and {Kokorev}, V. and {Le F{\`e}vre}, O. and {Lilly}, S. and {Masters}, D. and {Magdis}, G. and {Mehta}, V. and {Peng}, Y. and {Riechers}, D.~A. and {Salvato}, M. and {Sawicki}, M. and {Scarlata}, C. and {Scoville}, N. and {Shirley}, R. and {Silverman}, J.~D. and {Sneppen}, A. and {Smolc̆i{\'c}}, V. and {Steinhardt}, C. and {Stern}, D. and {Tanaka}, M. and {Taniguchi}, Y. and {Teplitz}, H.~I. and {Vaccari}, M. and {Wang}, W. -H. and {Zamorani}, G.},
        title = "{COSMOS2020: A Panchromatic View of the Universe to z 10 from Two Complementary Catalogs}",
      journal = {\apjs},
     keywords = {205, 1671, 594, 734, 1234, 1145, 1043, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2022,
        month = jan,
       volume = {258},
       number = {1},
          eid = {11},
        pages = {11},
          doi = {10.3847/1538-4365/ac3078},
archivePrefix = {arXiv},
       eprint = {2110.13923},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJS..258...11W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Weaver2021_farmer,
       author = {{Weaver}, John R. and {Zalesky}, L. and {Toft}, S.},
        title = "{The Farmer: some subtitle here}",
      journal = {\apjs},
     keywords = {catalogs; galaxies: evolution; galaxies: high-redshift; galaxies: photometry; methdods: observational; techniques: photometric},
         year = "in prep.",
        month = oct,
       volume = {30},
          eid = {e052},
        pages = {e052},
          doi = {10.1017/pasa.2013.31},
}

@ARTICLE{Bethermin2017,
       author = {{B{\'e}thermin}, Matthieu and {Wu}, Hao-Yi and {Lagache}, Guilaine and {Davidzon}, Iary and {Ponthieu}, Nicolas and {Cousin}, Morgane and {Wang}, Lingyu and {Dor{\'e}}, Olivier and {Daddi}, Emanuele and {Lapi}, Andrea},
        title = "{The impact of clustering and angular resolution on far-infrared and millimeter continuum observations}",
      journal = {\aap},
     keywords = {galaxies: statistics, galaxies: evolution, galaxies: star formation, galaxies: high-redshift, infrared: galaxies, submillimeter: galaxies, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2017,
        month = nov,
       volume = {607},
          eid = {A89},
        pages = {A89},
          doi = {10.1051/0004-6361/201730866},
archivePrefix = {arXiv},
       eprint = {1703.08795},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017A&A...607A..89B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Dubois2014,
       author = {{Dubois}, Y. and {Pichon}, C. and {Welker}, C. and {Le Borgne}, D. and {Devriendt}, J. and {Laigle}, C. and {Codis}, S. and {Pogosyan}, D. and {Arnouts}, S. and {Benabed}, K. and {Bertin}, E. and {Blaizot}, J. and {Bouchet}, F. and {Cardoso}, J. -F. and {Colombi}, S. and {de Lapparent}, V. and {Desjacques}, V. and {Gavazzi}, R. and {Kassin}, S. and {Kimm}, T. and {McCracken}, H. and {Milliard}, B. and {Peirani}, S. and {Prunet}, S. and {Rouberol}, S. and {Silk}, J. and {Slyz}, A. and {Sousbie}, T. and {Teyssier}, R. and {Tresse}, L. and {Treyer}, M. and {Vibert}, D. and {Volonteri}, M.},
        title = "{Dancing in the dark: galactic properties trace spin swings along the cosmic web}",
      journal = {\mnras},
     keywords = {methods: numerical, galaxies: evolution, galaxies: formation, galaxies: kinematics and dynamics, cosmology: theory, large-scale structure of Universe, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2014,
        month = oct,
       volume = {444},
       number = {2},
        pages = {1453-1468},
          doi = {10.1093/mnras/stu1227},
archivePrefix = {arXiv},
       eprint = {1402.1165},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014MNRAS.444.1453D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Gunn1972,
       author = {{Gunn}, James E. and {Gott}, J. Richard, III},
        title = "{On the Infall of Matter Into Clusters of Galaxies and Some Effects on Their Evolution}",
      journal = {\apj},
         year = 1972,
        month = aug,
       volume = {176},
        pages = {1},
          doi = {10.1086/151605},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1972ApJ...176....1G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Larson1980,
       author = {{Larson}, R.~B. and {Tinsley}, B.~M. and {Caldwell}, C.~N.},
        title = "{The evolution of disk galaxies and the origin of S0 galaxies}",
      journal = {\apj},
     keywords = {Disk Galaxies, Galactic Evolution, Spiral Galaxies, Digital Simulation, Galactic Structure, Gas Evolution, Stellar Evolution, Stellar Magnitude, Astrophysics},
         year = 1980,
        month = may,
       volume = {237},
        pages = {692-707},
          doi = {10.1086/157917},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1980ApJ...237..692L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Cole2001,
       author = {{Cole}, Shaun and {Norberg}, Peder and {Baugh}, Carlton M. and {Frenk}, Carlos S. and {Bland-Hawthorn}, Joss and {Bridges}, Terry and {Cannon}, Russell and {Colless}, Matthew and {Collins}, Chris and {Couch}, Warrick and {Cross}, Nicholas and {Dalton}, Gavin and {De Propris}, Roberto and {Driver}, Simon P. and {Efstathiou}, George and {Ellis}, Richard S. and {Glazebrook}, Karl and {Jackson}, Carole and {Lahav}, Ofer and {Lewis}, Ian and {Lumsden}, Stuart and {Maddox}, Steve and {Madgwick}, Darren and {Peacock}, John A. and {Peterson}, Bruce A. and {Sutherland}, Will and {Taylor}, Keith},
        title = "{The 2dF galaxy redshift survey: near-infrared galaxy luminosity functions}",
      journal = {\mnras},
     keywords = {SURVEYS, GALAXIES: LUMINOSITY FUNCTION, MASS FUNCTION, INFRARED: GALAXIES, Astrophysics},
         year = 2001,
        month = sep,
       volume = {326},
       number = {1},
        pages = {255-273},
          doi = {10.1046/j.1365-8711.2001.04591.x},
archivePrefix = {arXiv},
       eprint = {astro-ph/0012429},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2001MNRAS.326..255C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Steinhardt_tnse,
       author = {{Steinhardt}, Charles L. and {Weaver}, John R. and {Maxfield}, Jack and {Davidzon}, Iary and {Faisst}, Andreas L. and {Masters}, Dan and {Schemel}, Madeline and {Toft}, Sune},
        title = "{A Method to Distinguish Quiescent and Dusty Star-forming Galaxies with Machine Learning}",
      journal = {\apj},
     keywords = {1858, 293, 2040, 2016, 582, 1569, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2020,
        month = mar,
       volume = {891},
       number = {2},
          eid = {136},
        pages = {136},
          doi = {10.3847/1538-4357/ab76be},
archivePrefix = {arXiv},
       eprint = {2002.05729},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...891..136S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Arnouts2013,
       author = {{Arnouts}, S. and {Le Floc'h}, E. and {Chevallard}, J. and {Johnson}, B.~D. and {Ilbert}, O. and {Treyer}, M. and {Aussel}, H. and {Capak}, P. and {Sanders}, D.~B. and {Scoville}, N. and {McCracken}, H.~J. and {Milliard}, B. and {Pozzetti}, L. and {Salvato}, M.},
        title = "{Encoding of the infrared excess in the NUVrK color diagram for star-forming galaxies}",
      journal = {\aap},
     keywords = {infrared: galaxies, ultraviolet: galaxies, galaxies: evolution, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = oct,
       volume = {558},
          eid = {A67},
        pages = {A67},
          doi = {10.1051/0004-6361/201321768},
archivePrefix = {arXiv},
       eprint = {1309.0008},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013A&A...558A..67A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Nayyeri2017,
       author = {{Nayyeri}, H. and {Hemmati}, S. and {Mobasher}, B. and {Ferguson}, H.~C. and {Cooray}, A. and {Barro}, G. and {Faber}, S.~M. and {Dickinson}, M. and {Koekemoer}, A.~M. and {Peth}, M. and {Salvato}, M. and {Ashby}, M.~L.~N. and {Darvish}, B. and {Donley}, J. and {Durbin}, M. and {Finkelstein}, S. and {Fontana}, A. and {Grogin}, N.~A. and {Gruetzbauch}, R. and {Huang}, K. and {Khostovan}, A.~A. and {Kocevski}, D. and {Kodra}, D. and {Lee}, B. and {Newman}, J. and {Pacifici}, C. and {Pforr}, J. and {Stefanon}, M. and {Wiklind}, T. and {Willner}, S.~P. and {Wuyts}, S. and {Castellano}, M. and {Conselice}, C. and {Dolch}, T. and {Dunlop}, J.~S. and {Galametz}, A. and {Hathi}, N.~P. and {Lucas}, R.~A. and {Yan}, H.},
        title = "{CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field}",
      journal = {\apjs},
     keywords = {catalogs, galaxies: high-redshift, galaxies: photometry, methods: data analysis, techniques: image processing, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = jan,
       volume = {228},
       number = {1},
          eid = {7},
        pages = {7},
          doi = {10.3847/1538-4365/228/1/7},
archivePrefix = {arXiv},
       eprint = {1612.07364},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017ApJS..228....7N},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{malmquist1920,
       author = {{Malmquist}, K.~G.},
        title = "{Die Berechnung von Schiefheit und Exzess in der Verteilung der scheinbaren Magnitude}",
      journal = {Meddelanden fran Lunds Astronomiska Observatorium Serie I},
         year = 1920,
        month = aug,
       volume = {96},
        pages = {1-11},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1920MeLuF..96....1M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{malmquist1922,
       author = {{Malmquist}, K.~G.},
        title = "{On some relations in stellar statistics}",
      journal = {Meddelanden fran Lunds Astronomiska Observatorium Serie I},
         year = 1922,
        month = mar,
       volume = {100},
        pages = {1-52},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1922MeLuF.100....1M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Hogg1999,
       author = {{Hogg}, David W.},
        title = "{Distance measures in cosmology}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics},
         year = 1999,
        month = may,
          eid = {astro-ph/9905116},
        pages = {astro-ph/9905116},
archivePrefix = {arXiv},
       eprint = {astro-ph/9905116},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1999astro.ph..5116H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{schmidt1968,
       author = {{Schmidt}, Maarten},
        title = "{Space Distribution and Luminosity Functions of Quasi-Stellar Radio Sources}",
      journal = {\apj},
         year = 1968,
        month = feb,
       volume = {151},
        pages = {393},
          doi = {10.1086/149446},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1968ApJ...151..393S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{efstathiou1999,
       author = {{Efstathiou}, G. and {Bond}, J.~R.},
        title = "{Cosmic confusion: degeneracies among cosmological parameters derived from measurements of microwave background anisotropies}",
      journal = {\mnras},
     keywords = {COSMIC MICROWAVE BACKGROUND, COSMOLOGY: MISCELLANEOUS, Astrophysics},
         year = 1999,
        month = mar,
       volume = {304},
       number = {1},
        pages = {75-97},
          doi = {10.1046/j.1365-8711.1999.02274.x},
archivePrefix = {arXiv},
       eprint = {astro-ph/9807103},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1999MNRAS.304...75E},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{ilbert2005,
       author = {{Ilbert}, O. and {Tresse}, L. and {Zucca}, E. and {Bardelli}, S. and {Arnouts}, S. and {Zamorani}, G. and {Pozzetti}, L. and {Bottini}, D. and {Garilli}, B. and {Le Brun}, V. and {Le F{\`e}vre}, O. and {Maccagni}, D. and {Picat}, J. -P. and {Scaramella}, R. and {Scodeggio}, M. and {Vettolani}, G. and {Zanichelli}, A. and {Adami}, C. and {Arnaboldi}, M. and {Bolzonella}, M. and {Cappi}, A. and {Charlot}, S. and {Contini}, T. and {Foucaud}, S. and {Franzetti}, P. and {Gavignaud}, I. and {Guzzo}, L. and {Iovino}, A. and {McCracken}, H.~J. and {Marano}, B. and {Marinoni}, C. and {Mathez}, G. and {Mazure}, A. and {Meneux}, B. and {Merighi}, R. and {Paltani}, S. and {Pello}, R. and {Pollo}, A. and {Radovich}, M. and {Bondi}, M. and {Bongiorno}, A. and {Busarello}, G. and {Ciliegi}, P. and {Lamareille}, F. and {Mellier}, Y. and {Merluzzi}, P. and {Ripepi}, V. and {Rizzo}, D.},
        title = "{The VIMOS-VLT deep survey. Evolution of the galaxy luminosity function up to z = 2 in first epoch data}",
      journal = {\aap},
     keywords = {surveys, galaxies: evolution, galaxies: luminosity function, mass function, galaxies: statistics, Astrophysics},
         year = 2005,
        month = sep,
       volume = {439},
       number = {3},
        pages = {863-876},
          doi = {10.1051/0004-6361:20041961},
archivePrefix = {arXiv},
       eprint = {astro-ph/0409134},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2005A&A...439..863I},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{ilbert2004,
       author = {{Ilbert}, O. and {Tresse}, L. and {Arnouts}, S. and {Zucca}, E. and {Bardelli}, S. and {Zamorani}, G. and {Adami}, C. and {Cappi}, A. and {Garilli}, B. and {Le F{\`e}vre}, O. and {Maccagni}, D. and {Meneux}, B. and {Scaramella}, R. and {Scodeggio}, M. and {Vettolani}, G. and {Zanichelli}, A.},
        title = "{Bias in the estimation of global luminosity functions}",
      journal = {\mnras},
     keywords = {surveys, galaxies: luminosity function, Astrophysics},
         year = 2004,
        month = jun,
       volume = {351},
       number = {2},
        pages = {541-551},
          doi = {10.1111/j.1365-2966.2004.07796.x},
archivePrefix = {arXiv},
       eprint = {astro-ph/0402202},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2004MNRAS.351..541I},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{binggeli1998,
       author = {{Binggeli}, Bruno and {Jerjen}, Helmut},
        title = "{Is the shape of the luminosity profile of dwarf elliptical galaxies an useful distance indicator?}",
      journal = {\aap},
     keywords = {GALAXIES: DISTANCES AND REDSHIFTS, GALAXIES: ELLIPTICAL AND LENTICULAR, CD, GALAXIES: FUNDAMENTAL PARAMETERS, GALAXIES: PHOTOMETRY, Astrophysics},
         year = 1998,
        month = may,
       volume = {333},
        pages = {17-26},
archivePrefix = {arXiv},
       eprint = {astro-ph/9704027},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1998A&A...333...17B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{johnston2011,
       author = {{Johnston}, Russell},
        title = "{Shedding light on the galaxy luminosity function}",
      journal = {\aapr},
     keywords = {Galaxies: luminosity function, mass function, Methods: statistical, Cosmology: large-scale structure of the Universe, Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - Galaxy Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2011,
        month = aug,
       volume = {19},
          eid = {41},
        pages = {41},
          doi = {10.1007/s00159-011-0041-9},
archivePrefix = {arXiv},
       eprint = {1106.2039},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011A&ARv..19...41J},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{takeuchi2000,
       author = {{Takeuchi}, Tsutomu T.},
        title = "{Application of the Information Criterion to the Estimation of Galaxy Luminosity Function}",
      journal = {\apss},
     keywords = {Cosmology, galaxies: luminosity function, methods: statistical, Astrophysics},
         year = 2000,
        month = jan,
       volume = {271},
        pages = {213},
          doi = {10.1023/A:1002438524580},
archivePrefix = {arXiv},
       eprint = {astro-ph/9909324},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2000Ap&SS.271..213T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{weigel2016,
       author = {{Weigel}, Anna K. and {Schawinski}, Kevin and {Bruderer}, Claudio},
        title = "{Stellar mass functions: methods, systematics and results for the local Universe}",
      journal = {\mnras},
     keywords = {methods: data analysis, galaxies: general, galaxies: luminosity function, mass function, galaxies: statistics, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = jun,
       volume = {459},
       number = {2},
        pages = {2150-2187},
          doi = {10.1093/mnras/stw756},
archivePrefix = {arXiv},
       eprint = {1604.00008},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016MNRAS.459.2150W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Efstathiou1988,
       author = {{Efstathiou}, G. and {Ellis}, Richard S. and {Peterson}, Bruce A.},
        title = "{Analysis of a complete galaxy redshift survey. II. The field-galaxy luminosity function.}",
      journal = {\mnras},
     keywords = {Galactic Radiation, Luminous Intensity, Red Shift, Radiant Flux Density, Spatial Distribution, Astrophysics},
         year = 1988,
        month = may,
       volume = {232},
        pages = {431-461},
          doi = {10.1093/mnras/232.2.431},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1988MNRAS.232..431E},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{sandage1979,
       author = {{Sandage}, A. and {Tammann}, G.~A. and {Yahil}, A.},
        title = "{The velocity field of bright nearby galaxies. I. The variation of mean absolute magnitude with redshift for galaxies in a magnitude-limited sample.}",
      journal = {\apj},
     keywords = {Big Bang Cosmology, Galactic Radiation, Red Shift, Velocity Distribution, Distribution Functions, Histograms, Luminous Intensity, Magnitude, Maximum Likelihood Estimates, Astrophysics, Absolute Magnitudes:Galaxies, Galaxies:Hubble Diagram, Galaxies:Luminosity Function, Galaxies:Redshifts, Galaxies:Velocities},
         year = 1979,
        month = sep,
       volume = {232},
        pages = {352-364},
          doi = {10.1086/157295},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1979ApJ...232..352S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{schechter1976,
       author = {{Schechter}, P.},
        title = "{An analytic expression for the luminosity function for galaxies.}",
      journal = {\apj},
         year = 1976,
        month = jan,
       volume = {203},
        pages = {297-306},
          doi = {10.1086/154079},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1976ApJ...203..297S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Stefanon2021,
       author = {{Stefanon}, Mauro and {Labb{\'e}}, Ivo and {Oesch}, Pascal A. and {De Barros}, Stephane and {Gonzalez}, Valentino and {Bouwens}, Rychard J. and {Franx}, Marijn and {Illingworth}, Garth D. and {Holden}, Brad and {Magee}, Dan and {Smit}, Renske and {van Dokkum}, Pieter},
        title = "{The Spitzer/IRAC Legacy over the GOODS Fields: Full-depth 3.6, 4.5, 5.8, and 8.0 {\ensuremath{\mu}}m Mosaics and Photometry for >9000 Galaxies at z   3.5-10 from the GOODS Reionization Era Wide-area Treasury from Spitzer (GREATS)}",
      journal = {\apjs},
     keywords = {734, 611, 792, 1671},
         year = 2021,
        month = dec,
       volume = {257},
       number = {2},
          eid = {68},
        pages = {68},
          doi = {10.3847/1538-4365/ac2498},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJS..257...68S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}




@ARTICLE{Ucci2021,
       author = {{Ucci}, Graziano and {Dayal}, Pratika and {Hutter}, Anne and {Yepes}, Gustavo and {Gottl{\"o}ber}, Stefan and {Legrand}, Laurent and {Pentericci}, Laura and {Castellano}, Marco and {Choudhury}, Tirthankar Roy},
        title = "{Astraeus - II. Quantifying the impact of cosmic variance during the Epoch of Reionization}",
      journal = {\mnras},
     keywords = {galaxies: high-redshift, formation, evolution, star formation, luminosity function, cosmology: reionization, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = may,
          doi = {10.1093/mnras/stab1229},
archivePrefix = {arXiv},
       eprint = {2004.11096},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.tmp.1301U},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Trapp2020,
       author = {{Trapp}, A.~C. and {Furlanetto}, Steven R.},
        title = "{A flexible analytic model of cosmic variance in the first billion years}",
      journal = {\mnras},
     keywords = {methods: data analysis, galaxies: high-redshift, cosmology: theory, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = dec,
       volume = {499},
       number = {2},
        pages = {2401-2415},
          doi = {10.1093/mnras/staa2828},
archivePrefix = {arXiv},
       eprint = {2009.05059},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.499.2401T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{BluetidesBhowmick2020,
       author = {{Bhowmick}, Aklant K. and {Somerville}, Rachel S. and {Di Matteo}, Tiziana and {Wilkins}, Stephen and {Feng}, Yu and {Tenneti}, Ananth},
        title = "{Cosmic variance of z > 7 galaxies: prediction from BLUETIDES}",
      journal = {\mnras},
     keywords = {galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2020,
        month = jul,
       volume = {496},
       number = {1},
        pages = {754-766},
          doi = {10.1093/mnras/staa1605},
archivePrefix = {arXiv},
       eprint = {1908.02787},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.496..754B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{moster2011cosmic,
  title={A cosmic variance cookbook},
  author={Moster, Benjamin P and Somerville, Rachel S and Newman, Jeffrey A and Rix, Hans-Walter},
  journal={The Astrophysical Journal},
  volume={731},
  number={2},
  pages={113},
  year={2011},
  publisher={IOP Publishing}
}


@article{Driver2010CV_observational,
   title={Quantifying cosmic variance},
   volume={407},
   ISSN={0035-8711},
   url={http://dx.doi.org/10.1111/j.1365-2966.2010.17028.x},
   DOI={10.1111/j.1365-2966.2010.17028.x},
   number={4},
   journal={Monthly Notices of the Royal Astronomical Society},
   publisher={Oxford University Press (OUP)},
   author={Driver, Simon P. and Robotham, Aaron S. G.},
   year={2010},
   month={Sep},
   pages={2131–2140}
}

@ARTICLE{T+S_theory,
       author = {{Trenti}, M. and {Stiavelli}, M.},
        title = "{Cosmic Variance and Its Effect on the Luminosity Function Determination in Deep High-z Surveys}",
      journal = {\apj},
     keywords = {galaxies: high-redshift, galaxies: statistics, large-scale structure of universe, Astrophysics},
         year = 2008,
        month = apr,
       volume = {676},
       number = {2},
        pages = {767-780},
          doi = {10.1086/528674},
archivePrefix = {arXiv},
       eprint = {0712.0398},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2008ApJ...676..767T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Steinhardt2021,
       author = {{Steinhardt}, Charles L. and {Jespersen}, Christian Kragh and {Linzer}, Nora B.},
        title = "{Finding High-redshift Galaxies with JWST}",
      journal = {\apj},
     keywords = {734, 2007, 584, 902, 343, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = dec,
       volume = {923},
       number = {1},
          eid = {8},
        pages = {8},
          doi = {10.3847/1538-4357/ac2a2f},
archivePrefix = {arXiv},
       eprint = {2111.14865},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...923....8S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Dave2019_SIMBA,
       author = {{Dav{\'e}}, Romeel and {Angl{\'e}s-Alc{\'a}zar}, Daniel and {Narayanan}, Desika and {Li}, Qi and {Rafieferantsoa}, Mika H. and {Appleby}, Sarah},
        title = "{SIMBA: Cosmological simulations with black hole growth and feedback}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: formation, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2019,
        month = jun,
       volume = {486},
       number = {2},
        pages = {2827-2849},
          doi = {10.1093/mnras/stz937},
archivePrefix = {arXiv},
       eprint = {1901.10203},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.2827D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Furlong2015_EAGLE,
       author = {{Furlong}, M. and {Bower}, R.~G. and {Theuns}, T. and {Schaye}, J. and {Crain}, R.~A. and {Schaller}, M. and {Dalla Vecchia}, C. and {Frenk}, C.~S. and {McCarthy}, I.~G. and {Helly}, J. and {Jenkins}, A. and {Rosas-Guevara}, Y.~M.},
        title = "{Evolution of galaxy stellar masses and star formation rates in the EAGLE simulations}",
      journal = {\mnras},
     keywords = {galaxies: abundances, galaxies: evolution, galaxies: formation, galaxies: high-redshift, galaxies: star formation, Astrophysics - Astrophysics of Galaxies},
         year = 2015,
        month = jul,
       volume = {450},
       number = {4},
        pages = {4486-4504},
          doi = {10.1093/mnras/stv852},
archivePrefix = {arXiv},
       eprint = {1410.3485},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015MNRAS.450.4486F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Pillepich2018_ILLUSTRIS,
       author = {{Pillepich}, Annalisa and {Nelson}, Dylan and {Hernquist}, Lars and {Springel}, Volker and {Pakmor}, R{\"u}diger and {Torrey}, Paul and {Weinberger}, Rainer and {Genel}, Shy and {Naiman}, Jill P. and {Marinacci}, Federico and {Vogelsberger}, Mark},
        title = "{First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies}",
      journal = {\mnras},
     keywords = {methods: numerical, galaxies: clusters: general, galaxies: general, galaxies: groups: general, cosmology: theory, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2018,
        month = mar,
       volume = {475},
       number = {1},
        pages = {648-675},
          doi = {10.1093/mnras/stx3112},
archivePrefix = {arXiv},
       eprint = {1707.03406},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.475..648P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Lagos2018_SHARK,
       author = {{Lagos}, Claudia del P. and {Tobar}, Rodrigo J. and {Robotham}, Aaron S.~G. and {Obreschkow}, Danail and {Mitchell}, Peter D. and {Power}, Chris and {Elahi}, Pascal J.},
        title = "{Shark: introducing an open source, free, and flexible semi-analytic model of galaxy formation}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: formation, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = dec,
       volume = {481},
       number = {3},
        pages = {3573-3603},
          doi = {10.1093/mnras/sty2440},
archivePrefix = {arXiv},
       eprint = {1807.11180},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.481.3573L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Pacifici2015,
       author = {{Pacifici}, Camilla and {da Cunha}, Elisabete and {Charlot}, St{\'e}phane and {Rix}, Hans-Walter and {Fumagalli}, Mattia and {Wel}, Arjen van der and {Franx}, Marijn and {Maseda}, Michael V. and {van Dokkum}, Pieter G. and {Brammer}, Gabriel B. and {Momcheva}, Ivelina and {Skelton}, Rosalind E. and {Whitaker}, Katherine and {Leja}, Joel and {Lundgren}, Britt and {Kassin}, Susan A. and {Yi}, Sukyoung K.},
        title = "{On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7 < z < 2.8}",
      journal = {\mnras},
     keywords = {galaxies: fundamental parameters, galaxies: general, galaxies: statistics, galaxies: stellar content, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2015,
        month = feb,
       volume = {447},
       number = {1},
        pages = {786-805},
          doi = {10.1093/mnras/stu2447},
archivePrefix = {arXiv},
       eprint = {1411.5689},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015MNRAS.447..786P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Carnall2019,
       author = {{Carnall}, Adam C. and {Leja}, Joel and {Johnson}, Benjamin D. and {McLure}, Ross J. and {Dunlop}, James S. and {Conroy}, Charlie},
        title = "{How to Measure Galaxy Star Formation Histories. I. Parametric Models}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: fundamental parameters, galaxies: star formation, galaxies: statistics, galaxies: stellar content, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2019,
        month = mar,
       volume = {873},
       number = {1},
          eid = {44},
        pages = {44},
          doi = {10.3847/1538-4357/ab04a2},
archivePrefix = {arXiv},
       eprint = {1811.03635},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...873...44C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Leja2019,
       author = {{Leja}, Joel and {Carnall}, Adam C. and {Johnson}, Benjamin D. and {Conroy}, Charlie and {Speagle}, Joshua S.},
        title = "{How to Measure Galaxy Star Formation Histories. II. Nonparametric Models}",
      journal = {\apj},
     keywords = {galaxies: fundamental parameters, galaxies: star formation, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = may,
       volume = {876},
       number = {1},
          eid = {3},
        pages = {3},
          doi = {10.3847/1538-4357/ab133c},
archivePrefix = {arXiv},
       eprint = {1811.03637},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...876....3L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Shahidi2020,
       author = {{Shahidi}, Abtin and {Mobasher}, Bahram and {Nayyeri}, Hooshang and {Hemmati}, Shoubaneh and {Wiklind}, Tommy and {Chartab}, Nima and {Dickinson}, Mark and {Finkelstein}, Steven L. and {Pacifici}, Camilla and {Papovich}, Casey and {Ferguson}, Henry C. and {Fontana}, Adriano and {Giavalisco}, Mauro and {Koekemoer}, Anton and {Newman}, Jeffery and {Sattari}, Zahra and {Somerville}, Rachel},
        title = "{Selection of Massive Evolved Galaxies at 3 {\ensuremath{\leq}} z {\ensuremath{\leq}} 4.5 in the CANDELS Fields}",
      journal = {\apj},
     keywords = {734, 594, 573, 506, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = jul,
       volume = {897},
       number = {1},
          eid = {44},
        pages = {44},
          doi = {10.3847/1538-4357/ab96c5},
archivePrefix = {arXiv},
       eprint = {2005.12507},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...897...44S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Gehrels1986,
       author = {{Gehrels}, N.},
        title = "{Confidence Limits for Small Numbers of Events in Astrophysical Data}",
      journal = {\apj},
     keywords = {Astrophysics, Binomial Theorem, Confidence Limits, Data Processing, Poisson Density Functions, Approximation, Tables (Data), Astrophysics, NUMERICAL METHODS},
         year = 1986,
        month = apr,
       volume = {303},
        pages = {336},
          doi = {10.1086/164079},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1986ApJ...303..336G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Ebeling2003,
       author = {{Ebeling}, Harald},
        title = "{Improved approximations of Poissonian errors for high confidence levels}",
      journal = {\mnras},
     keywords = {methods: numerical, methods: statistical},
         year = 2003,
        month = apr,
       volume = {340},
       number = {4},
        pages = {1269-1278},
          doi = {10.1046/j.1365-8711.2003.06374.x},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2003MNRAS.340.1269E},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{SalpeterIMF,
       author = {{Salpeter}, Edwin E.},
        title = "{The Luminosity Function and Stellar Evolution.}",
      journal = {\apj},
         year = 1955,
        month = jan,
       volume = {121},
        pages = {161},
          doi = {10.1086/145971},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1955ApJ...121..161S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{ChabrierIMF,
       author = {{Chabrier}, Gilles},
        title = "{Galactic Stellar and Substellar Initial Mass Function}",
      journal = {\pasp},
     keywords = {Galaxies: Luminosity Function, Mass Function, Invited Reviews, Astrophysics},
         year = 2003,
        month = jul,
       volume = {115},
       number = {809},
        pages = {763-795},
          doi = {10.1086/376392},
archivePrefix = {arXiv},
       eprint = {astro-ph/0304382},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2003PASP..115..763C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Adams2021,
       author = {{Adams}, N.~J. and {Bowler}, R.~A.~A. and {Jarvis}, M.~J. and {H{\"a}u{\ss}ler}, B. and {Lagos}, C.~D.~P.},
        title = "{Evolution of the galaxy stellar mass function: evidence for an increasing M* from z = 2 to the present day}",
      journal = {\mnras},
     keywords = {galaxies: abundances, galaxies: evolution, galaxies: general, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = oct,
       volume = {506},
       number = {4},
        pages = {4933-4951},
          doi = {10.1093/mnras/stab1956},
archivePrefix = {arXiv},
       eprint = {2101.07182},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.506.4933A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Peng2015,
       author = {{Peng}, Y. and {Maiolino}, R. and {Cochrane}, R.},
        title = "{Strangulation as the primary mechanism for shutting down star formation in galaxies}",
      journal = {\nat},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2015,
        month = may,
       volume = {521},
       number = {7551},
        pages = {192-195},
          doi = {10.1038/nature14439},
archivePrefix = {arXiv},
       eprint = {1505.03143},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015Natur.521..192P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Varma2021,
       author = {{Varma}, S. and {Huertas-Company}, M. and {Pillepich}, A. and {Nelson}, D. and {Rodriguez-Gomez}, V. and {Dekel}, A. and {Faber}, S.~M. and {Iglesias-Navarro}, P. and {Koo}, D.~C. and {Primack}, J.},
        title = "{The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation}",
      journal = {\mnras},
     keywords = {galaxies: morphology, galaxies: evolution, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = nov,
          doi = {10.1093/mnras/stab3149},
archivePrefix = {arXiv},
       eprint = {2110.11989},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.tmp.2963V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Belli2019,
       author = {{Belli}, Sirio and {Newman}, Andrew B. and {Ellis}, Richard S.},
        title = "{MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II. Star Formation Histories and Galaxy Quenching}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, galaxies: stellar content, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = mar,
       volume = {874},
       number = {1},
          eid = {17},
        pages = {17},
          doi = {10.3847/1538-4357/ab07af},
archivePrefix = {arXiv},
       eprint = {1810.00008},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...874...17B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Suess2021,
       author = {{Suess}, Katherine A. and {Kriek}, Mariska and {Price}, Sedona H. and {Barro}, Guillermo},
        title = "{Dissecting the Size-Mass and {\ensuremath{\Sigma}}$_{1}$-Mass Relations at 1.0 < z < 2.5: Galaxy Mass Profiles and Color Gradients as a Function of Spectral Shape}",
      journal = {\apj},
     keywords = {Galaxy evolution, Galaxy structure, Galaxy quenching, Post-starburst galaxies, Green valley galaxies, Compact galaxies, 594, 622, 2040, 2176, 683, 285, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = jul,
       volume = {915},
       number = {2},
          eid = {87},
        pages = {87},
          doi = {10.3847/1538-4357/abf1e4},
archivePrefix = {arXiv},
       eprint = {2101.05820},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...915...87S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Bouche2010,
       author = {{Bouch{\'e}}, N. and {Dekel}, A. and {Genzel}, R. and {Genel}, S. and {Cresci}, G. and {F{\"o}rster Schreiber}, N.~M. and {Shapiro}, K.~L. and {Davies}, R.~I. and {Tacconi}, L.},
        title = "{The Impact of Cold Gas Accretion Above a Mass Floor on Galaxy Scaling Relations}",
      journal = {\apj},
     keywords = {cosmology: observations, galaxies: evolution, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2010,
        month = aug,
       volume = {718},
       number = {2},
        pages = {1001-1018},
          doi = {10.1088/0004-637X/718/2/1001},
archivePrefix = {arXiv},
       eprint = {0912.1858},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010ApJ...718.1001B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Balogh2000,
       author = {{Balogh}, Michael L. and {Navarro}, Julio F. and {Morris}, Simon L.},
        title = "{The Origin of Star Formation Gradients in Rich Galaxy Clusters}",
      journal = {\apj},
     keywords = {Galaxies: Clusters: General, Galaxies: Evolution, Galaxies: Stellar Content, Stars: Formation, Astrophysics},
         year = 2000,
        month = sep,
       volume = {540},
       number = {1},
        pages = {113-121},
          doi = {10.1086/309323},
archivePrefix = {arXiv},
       eprint = {astro-ph/0004078},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2000ApJ...540..113B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Torrey2014,
       author = {{Torrey}, Paul and {Vogelsberger}, Mark and {Genel}, Shy and {Sijacki}, Debora and {Springel}, Volker and {Hernquist}, Lars},
        title = "{A model for cosmological simulations of galaxy formation physics: multi-epoch validation}",
      journal = {\mnras},
     keywords = {methods: numerical, galaxies: evolution, galaxies: formation, cosmology: theory, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2014,
        month = mar,
       volume = {438},
       number = {3},
        pages = {1985-2004},
          doi = {10.1093/mnras/stt2295},
archivePrefix = {arXiv},
       eprint = {1305.4931},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014MNRAS.438.1985T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Moster2014,
       author = {{Moster}, Benjamin P. and {Macci{\`o}}, Andrea V. and {Somerville}, Rachel S.},
        title = "{Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky Way-like galaxies}",
      journal = {\mnras},
     keywords = {methods: numerical, Galaxy: evolution, galaxies: evolution, galaxies: interactions, galaxies: structure, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2014,
        month = jan,
       volume = {437},
       number = {2},
        pages = {1027-1044},
          doi = {10.1093/mnras/stt1702},
archivePrefix = {arXiv},
       eprint = {1210.5522},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014MNRAS.437.1027M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Moster2013,
       author = {{Moster}, Benjamin P. and {Naab}, Thorsten and {White}, Simon D.~M.},
        title = "{Galactic star formation and accretion histories from matching galaxies to dark matter haloes}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: high-redshift, galaxies: statistics, galaxies: stellar content, cosmology: theory, dark matter, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = feb,
       volume = {428},
       number = {4},
        pages = {3121-3138},
          doi = {10.1093/mnras/sts261},
archivePrefix = {arXiv},
       eprint = {1205.5807},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013MNRAS.428.3121M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Volonteri2016,
       author = {{Volonteri}, Marta and {Reines}, Amy E.},
        title = "{Inferences on the Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the High-redshift Universe}",
      journal = {\apjl},
     keywords = {galaxies: active, galaxies: evolution, galaxies: high-redshift, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2016,
        month = mar,
       volume = {820},
       number = {1},
          eid = {L6},
        pages = {L6},
          doi = {10.3847/2041-8205/820/1/L6},
archivePrefix = {arXiv},
       eprint = {1602.05711},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016ApJ...820L...6V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Marchesini2009,
       author = {{Marchesini}, Danilo and {van Dokkum}, Pieter G. and {F{\"o}rster Schreiber}, Natascha M. and {Franx}, Marijn and {Labb{\'e}}, Ivo and {Wuyts}, Stijn},
        title = "{The Evolution of the Stellar Mass Function of Galaxies from z = 4.0 and the First Comprehensive Analysis of its Uncertainties: Evidence for Mass-Dependent Evolution}",
      journal = {\apj},
     keywords = {galaxies: distances and redshifts, galaxies: evolution, galaxies: formation, galaxies: fundamental parameters, galaxies: high-redshift, galaxies: luminosity function, mass function, galaxies: stellar content, infrared: galaxies, Astrophysics},
         year = 2009,
        month = aug,
       volume = {701},
       number = {2},
        pages = {1765-1796},
          doi = {10.1088/0004-637X/701/2/1765},
archivePrefix = {arXiv},
       eprint = {0811.1773},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009ApJ...701.1765M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}




@ARTICLE{Henriques2015,
       author = {{Henriques}, Bruno M.~B. and {White}, Simon D.~M. and {Thomas}, Peter A. and {Angulo}, Raul and {Guo}, Qi and {Lemson}, Gerard and {Springel}, Volker and {Overzier}, Roderik},
        title = "{Galaxy formation in the Planck cosmology - I. Matching the observed evolution of star formation rates, colours and stellar masses}",
      journal = {\mnras},
     keywords = {methods: analytical, methods: statistical, galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2015,
        month = aug,
       volume = {451},
       number = {3},
        pages = {2663-2680},
          doi = {10.1093/mnras/stv705},
archivePrefix = {arXiv},
       eprint = {1410.0365},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015MNRAS.451.2663H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{McLeod2021,
       author = {{McLeod}, D.~J. and {McLure}, R.~J. and {Dunlop}, J.~S. and {Cullen}, F. and {Carnall}, A.~C. and {Duncan}, K.},
        title = "{The evolution of the galaxy stellar-mass function over the last 12 billion years from a combination of ground-based and HST surveys}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = may,
       volume = {503},
       number = {3},
        pages = {4413-4435},
          doi = {10.1093/mnras/stab731},
archivePrefix = {arXiv},
       eprint = {2009.03176},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.503.4413M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Behroozi2019,
       author = {{Behroozi}, Peter and {Wechsler}, Risa H. and {Hearin}, Andrew P. and {Conroy}, Charlie},
        title = "{UNIVERSEMACHINE: The correlation between galaxy growth and dark matter halo assembly from z = 0-10}",
      journal = {\mnras},
     keywords = {galaxies: formation, galaxies: haloes, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = sep,
       volume = {488},
       number = {3},
        pages = {3143-3194},
          doi = {10.1093/mnras/stz1182},
archivePrefix = {arXiv},
       eprint = {1806.07893},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.488.3143B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Gonzalez2011,
       author = {{Gonz{\'a}lez}, Valentino and {Labb{\'e}}, Ivo and {Bouwens}, Rychard J. and {Illingworth}, Garth and {Franx}, Marijn and {Kriek}, Mariska},
        title = "{Evolution of Galaxy Stellar Mass Functions, Mass Densities, and Mass-to-light Ratios from z \raisebox{-0.5ex}\textasciitilde 7 to z \raisebox{-0.5ex}\textasciitilde 4}",
      journal = {\apjl},
     keywords = {galaxies: evolution, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2011,
        month = jul,
       volume = {735},
       number = {2},
          eid = {L34},
        pages = {L34},
          doi = {10.1088/2041-8205/735/2/L34},
archivePrefix = {arXiv},
       eprint = {1008.3901},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJ...735L..34G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Wright2018,
       author = {{Wright}, A.~H. and {Driver}, S.~P. and {Robotham}, A.~S.~G.},
        title = "{GAMA/G10-COSMOS/3D-HST: Evolution of the galaxy stellar mass function over 12.5 Gyr}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: luminosity function, mass function, galaxies: stellar content, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = nov,
       volume = {480},
       number = {3},
        pages = {3491-3502},
          doi = {10.1093/mnras/sty2136},
archivePrefix = {arXiv},
       eprint = {1808.01754},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.3491W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Santini2021,
       author = {{Santini}, P. and {Castellano}, M. and {Merlin}, E. and {Fontana}, A. and {Fortuni}, F. and {Kodra}, D. and {Magnelli}, B. and {Menci}, N. and {Calabr{\`o}}, A. and {Lovell}, C.~C. and {Pentericci}, L. and {Testa}, V. and {Wilkins}, S.~M.},
        title = "{The emergence of passive galaxies in the early Universe}",
      journal = {\aap},
     keywords = {galaxies: evolution, galaxies: high-redshift, galaxies: luminosity function, mass function, methods: data analysis, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = aug,
       volume = {652},
          eid = {A30},
        pages = {A30},
          doi = {10.1051/0004-6361/202039738},
archivePrefix = {arXiv},
       eprint = {2011.10584},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...652A..30S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Tinker2008,
       author = {{Tinker}, Jeremy and {Kravtsov}, Andrey V. and {Klypin}, Anatoly and {Abazajian}, Kevork and {Warren}, Michael and {Yepes}, Gustavo and {Gottl{\"o}ber}, Stefan and {Holz}, Daniel E.},
        title = "{Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality}",
      journal = {\apj},
     keywords = {cosmology: theory, large-scale structure of universe, methods: numerical, Astrophysics},
         year = 2008,
        month = dec,
       volume = {688},
       number = {2},
        pages = {709-728},
          doi = {10.1086/591439},
archivePrefix = {arXiv},
       eprint = {0803.2706},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2008ApJ...688..709T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Planck2018,
       author = {{Planck Collaboration} and {Aghanim}, N. and {Akrami}, Y. and {Ashdown}, M. and {Aumont}, J. and {Baccigalupi}, C. and {Ballardini}, M. and {Banday}, A.~J. and {Barreiro}, R.~B. and {Bartolo}, N. and {Basak}, S. and {Battye}, R. and {Benabed}, K. and {Bernard}, J. -P. and {Bersanelli}, M. and {Bielewicz}, P. and {Bock}, J.~J. and {Bond}, J.~R. and {Borrill}, J. and {Bouchet}, F.~R. and {Boulanger}, F. and {Bucher}, M. and {Burigana}, C. and {Butler}, R.~C. and {Calabrese}, E. and {Cardoso}, J. -F. and {Carron}, J. and {Challinor}, A. and {Chiang}, H.~C. and {Chluba}, J. and {Colombo}, L.~P.~L. and {Combet}, C. and {Contreras}, D. and {Crill}, B.~P. and {Cuttaia}, F. and {de Bernardis}, P. and {de Zotti}, G. and {Delabrouille}, J. and {Delouis}, J. -M. and {Di Valentino}, E. and {Diego}, J.~M. and {Dor{\'e}}, O. and {Douspis}, M. and {Ducout}, A. and {Dupac}, X. and {Dusini}, S. and {Efstathiou}, G. and {Elsner}, F. and {En{\ss}lin}, T.~A. and {Eriksen}, H.~K. and {Fantaye}, Y. and {Farhang}, M. and {Fergusson}, J. and {Fernandez-Cobos}, R. and {Finelli}, F. and {Forastieri}, F. and {Frailis}, M. and {Fraisse}, A.~A. and {Franceschi}, E. and {Frolov}, A. and {Galeotta}, S. and {Galli}, S. and {Ganga}, K. and {G{\'e}nova-Santos}, R.~T. and {Gerbino}, M. and {Ghosh}, T. and {Gonz{\'a}lez-Nuevo}, J. and {G{\'o}rski}, K.~M. and {Gratton}, S. and {Gruppuso}, A. and {Gudmundsson}, J.~E. and {Hamann}, J. and {Handley}, W. and {Hansen}, F.~K. and {Herranz}, D. and {Hildebrandt}, S.~R. and {Hivon}, E. and {Huang}, Z. and {Jaffe}, A.~H. and {Jones}, W.~C. and {Karakci}, A. and {Keih{\"a}nen}, E. and {Keskitalo}, R. and {Kiiveri}, K. and {Kim}, J. and {Kisner}, T.~S. and {Knox}, L. and {Krachmalnicoff}, N. and {Kunz}, M. and {Kurki-Suonio}, H. and {Lagache}, G. and {Lamarre}, J. -M. and {Lasenby}, A. and {Lattanzi}, M. and {Lawrence}, C.~R. and {Le Jeune}, M. and {Lemos}, P. and {Lesgourgues}, J. and {Levrier}, F. and {Lewis}, A. and {Liguori}, M. and {Lilje}, P.~B. and {Lilley}, M. and {Lindholm}, V. and {L{\'o}pez-Caniego}, M. and {Lubin}, P.~M. and {Ma}, Y. -Z. and {Mac{\'\i}as-P{\'e}rez}, J.~F. and {Maggio}, G. and {Maino}, D. and {Mandolesi}, N. and {Mangilli}, A. and {Marcos-Caballero}, A. and {Maris}, M. and {Martin}, P.~G. and {Martinelli}, M. and {Mart{\'\i}nez-Gonz{\'a}lez}, E. and {Matarrese}, S. and {Mauri}, N. and {McEwen}, J.~D. and {Meinhold}, P.~R. and {Melchiorri}, A. and {Mennella}, A. and {Migliaccio}, M. and {Millea}, M. and {Mitra}, S. and {Miville-Desch{\^e}nes}, M. -A. and {Molinari}, D. and {Montier}, L. and {Morgante}, G. and {Moss}, A. and {Natoli}, P. and {N{\o}rgaard-Nielsen}, H.~U. and {Pagano}, L. and {Paoletti}, D. and {Partridge}, B. and {Patanchon}, G. and {Peiris}, H.~V. and {Perrotta}, F. and {Pettorino}, V. and {Piacentini}, F. and {Polastri}, L. and {Polenta}, G. and {Puget}, J. -L. and {Rachen}, J.~P. and {Reinecke}, M. and {Remazeilles}, M. and {Renzi}, A. and {Rocha}, G. and {Rosset}, C. and {Roudier}, G. and {Rubi{\~n}o-Mart{\'\i}n}, J.~A. and {Ruiz-Granados}, B. and {Salvati}, L. and {Sandri}, M. and {Savelainen}, M. and {Scott}, D. and {Shellard}, E.~P.~S. and {Sirignano}, C. and {Sirri}, G. and {Spencer}, L.~D. and {Sunyaev}, R. and {Suur-Uski}, A. -S. and {Tauber}, J.~A. and {Tavagnacco}, D. and {Tenti}, M. and {Toffolatti}, L. and {Tomasi}, M. and {Trombetti}, T. and {Valenziano}, L. and {Valiviita}, J. and {Van Tent}, B. and {Vibert}, L. and {Vielva}, P. and {Villa}, F. and {Vittorio}, N. and {Wandelt}, B.~D. and {Wehus}, I.~K. and {White}, M. and {White}, S.~D.~M. and {Zacchei}, A. and {Zonca}, A.},
        title = "{Planck 2018 results. VI. Cosmological parameters}",
      journal = {\aap},
     keywords = {cosmic background radiation, cosmological parameters, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2020,
        month = sep,
       volume = {641},
          eid = {A6},
        pages = {A6},
          doi = {10.1051/0004-6361/201833910},
archivePrefix = {arXiv},
       eprint = {1807.06209},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...641A...6P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Steinhardt2016,
       author = {{Steinhardt}, Charles. L. and {Capak}, Peter and {Masters}, Dan and {Speagle}, Josh S.},
        title = "{The Impossibly Early Galaxy Problem}",
      journal = {\apj},
     keywords = {dark matter, galaxies: evolution, galaxies: formation, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = jun,
       volume = {824},
       number = {1},
          eid = {21},
        pages = {21},
          doi = {10.3847/0004-637X/824/1/21},
archivePrefix = {arXiv},
       eprint = {1506.01377},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016ApJ...824...21S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Behroozi2018,
       author = {{Behroozi}, Peter and {Silk}, Joseph},
        title = "{The most massive galaxies and black holes allowed by {\ensuremath{\Lambda}}CDM}",
      journal = {\mnras},
     keywords = {galaxies: haloes, early Universe, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = jul,
       volume = {477},
       number = {4},
        pages = {5382-5387},
          doi = {10.1093/mnras/sty945},
archivePrefix = {arXiv},
       eprint = {1609.04402},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.477.5382B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Bolzonella2010,
       author = {{Bolzonella}, M. and {Kova{\v{c}}}, K. and {Pozzetti}, L. and {Zucca}, E. and {Cucciati}, O. and {Lilly}, S.~J. and {Peng}, Y. and {Iovino}, A. and {Zamorani}, G. and {Vergani}, D. and {Tasca}, L.~A.~M. and {Lamareille}, F. and {Oesch}, P. and {Caputi}, K. and {Kampczyk}, P. and {Bardelli}, S. and {Maier}, C. and {Abbas}, U. and {Knobel}, C. and {Scodeggio}, M. and {Carollo}, C.~M. and {Contini}, T. and {Kneib}, J. -P. and {Le F{\`e}vre}, O. and {Mainieri}, V. and {Renzini}, A. and {Bongiorno}, A. and {Coppa}, G. and {de la Torre}, S. and {de Ravel}, L. and {Franzetti}, P. and {Garilli}, B. and {Le Borgne}, J. -F. and {Le Brun}, V. and {Mignoli}, M. and {Pell{\'o}}, R. and {Perez-Montero}, E. and {Ricciardelli}, E. and {Silverman}, J.~D. and {Tanaka}, M. and {Tresse}, L. and {Bottini}, D. and {Cappi}, A. and {Cassata}, P. and {Cimatti}, A. and {Guzzo}, L. and {Koekemoer}, A.~M. and {Leauthaud}, A. and {Maccagni}, D. and {Marinoni}, C. and {McCracken}, H.~J. and {Memeo}, P. and {Meneux}, B. and {Porciani}, C. and {Scaramella}, R. and {Aussel}, H. and {Capak}, P. and {Halliday}, C. and {Ilbert}, O. and {Kartaltepe}, J. and {Salvato}, M. and {Sanders}, D. and {Scarlata}, C. and {Scoville}, N. and {Taniguchi}, Y. and {Thompson}, D.},
        title = "{Tracking the impact of environment on the galaxy stellar mass function up to z \raisebox{-0.5ex}\textasciitilde 1 in the 10 k zCOSMOS sample}",
      journal = {\aap},
     keywords = {cosmology: observations, galaxies: evolution, galaxies: fundamental parameters, galaxies: luminosity function, mass function, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2010,
        month = dec,
       volume = {524},
          eid = {A76},
        pages = {A76},
          doi = {10.1051/0004-6361/200912801},
archivePrefix = {arXiv},
       eprint = {0907.0013},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010A&A...524A..76B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Davidzon2016,
       author = {{Davidzon}, I. and {Cucciati}, O. and {Bolzonella}, M. and {De Lucia}, G. and {Zamorani}, G. and {Arnouts}, S. and {Moutard}, T. and {Ilbert}, O. and {Garilli}, B. and {Scodeggio}, M. and {Guzzo}, L. and {Abbas}, U. and {Adami}, C. and {Bel}, J. and {Bottini}, D. and {Branchini}, E. and {Cappi}, A. and {Coupon}, J. and {de la Torre}, S. and {Di Porto}, C. and {Fritz}, A. and {Franzetti}, P. and {Fumana}, M. and {Granett}, B.~R. and {Guennou}, L. and {Iovino}, A. and {Krywult}, J. and {Le Brun}, V. and {Le F{\`e}vre}, O. and {Maccagni}, D. and {Ma{\l}ek}, K. and {Marulli}, F. and {McCracken}, H.~J. and {Mellier}, Y. and {Moscardini}, L. and {Polletta}, M. and {Pollo}, A. and {Tasca}, L.~A.~M. and {Tojeiro}, R. and {Vergani}, D. and {Zanichelli}, A.},
        title = "{The VIMOS Public Extragalactic Redshift Survey (VIPERS). Environmental effects shaping the galaxy stellar mass function}",
      journal = {\aap},
     keywords = {galaxies: evolution, galaxies: statistics, galaxies: interactions, large-scale structure of Universe, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = feb,
       volume = {586},
          eid = {A23},
        pages = {A23},
          doi = {10.1051/0004-6361/201527129},
archivePrefix = {arXiv},
       eprint = {1511.01145},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016A&A...586A..23D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Eddington1913,
       author = {{Eddington}, A.~S.},
        title = "{On a formula for correcting statistics for the effects of a known error of observation}",
      journal = {\mnras},
         year = 1913,
        month = mar,
       volume = {73},
        pages = {359-360},
          doi = {10.1093/mnras/73.5.359},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1913MNRAS..73..359E},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{Cirasuolo2012,
       author = {{Cirasuolo}, M. and {Afonso}, J. and {Bender}, R. and {Bonifacio}, P. and {Evans}, C. and {Kaper}, L. and {Oliva}, Ernesto and {Vanzi}, Leonardo and {Abreu}, Manuel and {Atad-Ettedgui}, Eli and {Babusiaux}, Carine and {Bauer}, Franz E. and {Best}, Philip and {Bezawada}, Naidu and {Bryson}, Ian R. and {Cabral}, Alexandre and {Caputi}, Karina and {Centrone}, Mauro and {Chemla}, Fanny and {Cimatti}, Andrea and {Cioni}, Maria-Rosa and {Clementini}, Gisella and {Coelho}, Jo{\~a}o. and {Daddi}, Emanuele and {Dunlop}, James S. and {Feltzing}, Sofia and {Ferguson}, Annette and {Flores}, Hector and {Fontana}, Adriano and {Fynbo}, Johan and {Garilli}, Bianca and {Glauser}, Adrian M. and {Guinouard}, Isabelle and {Hammer}, Jean-Fran{\c{c}}ois and {Hastings}, Peter R. and {Hess}, Hans-Joachim and {Ivison}, Rob J. and {Jagourel}, Pascal and {Jarvis}, Matt and {Kauffman}, G. and {Lawrence}, A. and {Lee}, D. and {Li Causi}, G. and {Lilly}, S. and {Lorenzetti}, D. and {Maiolino}, R. and {Mannucci}, F. and {McLure}, R. and {Minniti}, D. and {Montgomery}, D. and {Muschielok}, B. and {Nandra}, K. and {Navarro}, R. and {Norberg}, P. and {Origlia}, L. and {Padilla}, N. and {Peacock}, J. and {Pedicini}, F. and {Pentericci}, L. and {Pragt}, J. and {Puech}, M. and {Randich}, S. and {Renzini}, A. and {Ryde}, N. and {Rodrigues}, M. and {Royer}, F. and {Saglia}, R. and {S{\'a}nchez}, A. and {Schnetler}, H. and {Sobral}, D. and {Speziali}, R. and {Todd}, S. and {Tolstoy}, E. and {Torres}, M. and {Venema}, L. and {Vitali}, F. and {Wegner}, M. and {Wells}, M. and {Wild}, V. and {Wright}, G.},
        title = "{MOONS: a multi-object optical and near-infrared spectrograph for the VLT}",
     keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
    booktitle = {Ground-based and Airborne Instrumentation for Astronomy IV},
         year = 2012,
       editor = {{McLean}, Ian S. and {Ramsay}, Suzanne K. and {Takami}, Hideki},
       series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
       volume = {8446},
        month = sep,
          eid = {84460S},
        pages = {84460S},
          doi = {10.1117/12.925871},
archivePrefix = {arXiv},
       eprint = {1208.5780},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012SPIE.8446E..0SC},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{Tamura2016,
       author = {{Tamura}, Naoyuki and {Takato}, Naruhisa and {Shimono}, Atsushi and {Moritani}, Yuki and {Yabe}, Kiyoto and {Ishizuka}, Yuki and {Ueda}, Akitoshi and {Kamata}, Yukiko and {Aghazarian}, Hrand and {Arnouts}, St{\'e}phane and {Barban}, Gabriel and {Barkhouser}, Robert H. and {Borges}, Renato C. and {Braun}, David F. and {Carr}, Michael A. and {Chabaud}, Pierre-Yves and {Chang}, Yin-Chang and {Chen}, Hsin-Yo and {Chiba}, Masashi and {Chou}, Richard C.~Y. and {Chu}, You-Hua and {Cohen}, Judith and {de Almeida}, Rodrigo P. and {de Oliveira}, Antonio C. and {de Oliveira}, Ligia S. and {Dekany}, Richard G. and {Dohlen}, Kjetil and {dos Santos}, Jesulino B. and {dos Santos}, Leandro H. and {Ellis}, Richard and {Fabricius}, Maximilian and {Ferrand}, Didier and {Ferreira}, D{\'e}cio and {Golebiowski}, Mirek and {Greene}, Jenny E. and {Gross}, Johannes and {Gunn}, James E. and {Hammond}, Randolph and {Harding}, Albert and {Hart}, Murdock and {Heckman}, Timothy M. and {Hirata}, Christopher M. and {Ho}, Paul and {Hope}, Stephen C. and {Hovland}, Larry and {Hsu}, Shu-Fu and {Hu}, Yen-Shan and {Huang}, Ping-Jie and {Jaquet}, Marc and {Jing}, Yipeng and {Karr}, Jennifer and {Kimura}, Masahiko and {King}, Matthew E. and {Komatsu}, Eiichiro and {Le Brun}, Vincent and {Le F{\`e}vre}, Olivier and {Le Fur}, Arnaud and {Le Mignant}, David and {Ling}, Hung-Hsu and {Loomis}, Craig P. and {Lupton}, Robert H. and {Madec}, Fabrice and {Mao}, Peter and {Marrara}, Lucas S. and {Mendes de Oliveira}, Claudia and {Minowa}, Yosuke and {Morantz}, Chaz and {Murayama}, Hitoshi and {Murray}, Graham J. and {Ohyama}, Youichi and {Orndorff}, Joseph and {Pascal}, Sandrine and {Pereira}, Jefferson M. and {Reiley}, Daniel and {Reinecke}, Martin and {Ritter}, Andreas and {Roberts}, Mitsuko and {Schwochert}, Mark A. and {Seiffert}, Michael D. and {Smee}, Stephen A. and {Sodre}, Laerte and {Spergel}, David N. and {Steinkraus}, Aaron J. and {Strauss}, Michael A. and {Surace}, Christian and {Suto}, Yasushi and {Suzuki}, Nao and {Swinbank}, John and {Tait}, Philip J. and {Takada}, Masahiro and {Tamura}, Tomonori and {Tanaka}, Yoko and {Tresse}, Laurence and {Verducci}, Orlando and {Vibert}, Didier and {Vidal}, Clement and {Wang}, Shiang-Yu and {Wen}, Chih-Yi and {Yan}, Chi-Hung and {Yasuda}, Naoki},
        title = "{Prime Focus Spectrograph (PFS) for the Subaru telescope: overview, recent progress, and future perspectives}",
     keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
    booktitle = {Ground-based and Airborne Instrumentation for Astronomy VI},
         year = 2016,
       editor = {{Evans}, Christopher J. and {Simard}, Luc and {Takami}, Hideki},
       series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
       volume = {9908},
        month = aug,
          eid = {99081M},
        pages = {99081M},
          doi = {10.1117/12.2232103},
archivePrefix = {arXiv},
       eprint = {1608.01075},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016SPIE.9908E..1MT},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Neistein2006,
       author = {{Neistein}, Eyal and {van den Bosch}, Frank C. and {Dekel}, Avishai},
        title = "{Natural downsizing in hierarchical galaxy formation}",
      journal = {\mnras},
     keywords = {galaxies: elliptical and lenticular, cD, galaxies: haloes, cosmology: theory, dark matter, Astrophysics},
         year = 2006,
        month = oct,
       volume = {372},
       number = {2},
        pages = {933-948},
          doi = {10.1111/j.1365-2966.2006.10918.x},
archivePrefix = {arXiv},
       eprint = {astro-ph/0605045},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2006MNRAS.372..933N},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Cowie1996,
       author = {{Cowie}, Lennox L. and {Songaila}, Antoinette and {Hu}, Esther M. and {Cohen}, J.~G.},
        title = "{New Insight on Galaxy Formation and Evolution From Keck Spectroscopy of the Hawaii Deep Fields}",
      journal = {\aj},
     keywords = {GALAXIES: FORMATION, GALAXIES: EVOLUTION, SURVEYS, Astrophysics},
         year = 1996,
        month = sep,
       volume = {112},
        pages = {839},
          doi = {10.1086/118058},
archivePrefix = {arXiv},
       eprint = {astro-ph/9606079},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1996AJ....112..839C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{McConachie2021,
       author = {{McConachie}, Ian and {Wilson}, Gillian and {Forrest}, Ben and {Marsan}, Z. Cemile and {Muzzin}, Adam and {Cooper}, M.~C. and {Annunziatella}, Marianna and {Marchesini}, Danilo and {Chan}, Jeffrey C.~C. and {Gomez}, Percy and {Abdullah}, Mohamed H. and {Saracco}, Paolo and {Nantais}, Julie},
        title = "{Spectroscopic Confirmation of a Protocluster at $z=3.37$ with a High Fraction of Quiescent Galaxies}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = sep,
          eid = {arXiv:2109.07696},
        pages = {arXiv:2109.07696},
archivePrefix = {arXiv},
       eprint = {2109.07696},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210907696M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Harikane2016,
       author = {{Harikane}, Yuichi and {Ouchi}, Masami and {Ono}, Yoshiaki and {More}, Surhud and {Saito}, Shun and {Lin}, Yen-Ting and {Coupon}, Jean and {Shimasaku}, Kazuhiro and {Shibuya}, Takatoshi and {Price}, Paul A. and {Lin}, Lihwai and {Hsieh}, Bau-Ching and {Ishigaki}, Masafumi and {Komiyama}, Yutaka and {Silverman}, John and {Takata}, Tadafumi and {Tamazawa}, Hiroko and {Toshikawa}, Jun},
        title = "{Evolution of Stellar-to-Halo Mass Ratio at z = 0 - 7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2016,
        month = apr,
       volume = {821},
       number = {2},
          eid = {123},
        pages = {123},
          doi = {10.3847/0004-637X/821/2/123},
archivePrefix = {arXiv},
       eprint = {1511.07873},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016ApJ...821..123H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Song2016,
       author = {{Song}, Mimi and {Finkelstein}, Steven L. and {Ashby}, Matthew L.~N. and {Grazian}, A. and {Lu}, Yu and {Papovich}, Casey and {Salmon}, Brett and {Somerville}, Rachel S. and {Dickinson}, Mark and {Duncan}, K. and {Faber}, Sandy M. and {Fazio}, Giovanni G. and {Ferguson}, Henry C. and {Fontana}, Adriano and {Guo}, Yicheng and {Hathi}, Nimish and {Lee}, Seong-Kook and {Merlin}, Emiliano and {Willner}, S.~P.},
        title = "{The Evolution of the Galaxy Stellar Mass Function at z = 4-8: A Steepening Low-mass-end Slope with Increasing Redshift}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, galaxies: luminosity function, mass function, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = jul,
       volume = {825},
       number = {1},
          eid = {5},
        pages = {5},
          doi = {10.3847/0004-637X/825/1/5},
archivePrefix = {arXiv},
       eprint = {1507.05636},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016ApJ...825....5S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Conroy2009,
       author = {{Conroy}, Charlie and {Gunn}, James E. and {White}, Martin},
        title = "{The Propagation of Uncertainties in Stellar Population Synthesis Modeling. I. The Relevance of Uncertain Aspects of Stellar Evolution and the Initial Mass Function to the Derived Physical Properties of Galaxies}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: stellar content, stars: evolution, Astrophysics},
         year = 2009,
        month = jul,
       volume = {699},
       number = {1},
        pages = {486-506},
          doi = {10.1088/0004-637X/699/1/486},
archivePrefix = {arXiv},
       eprint = {0809.4261},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009ApJ...699..486C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Conroy2010,
       author = {{Conroy}, Charlie and {Gunn}, James E.},
        title = "{The Propagation of Uncertainties in Stellar Population Synthesis Modeling. III. Model Calibration, Comparison, and Evaluation}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: stellar content, stars: evolution, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2010,
        month = apr,
       volume = {712},
       number = {2},
        pages = {833-857},
          doi = {10.1088/0004-637X/712/2/833},
archivePrefix = {arXiv},
       eprint = {0911.3151},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010ApJ...712..833C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Vulcani2013,
       author = {{Vulcani}, B. and {Poggianti}, B.~M. and {Oemler}, A. and {Dressler}, A. and {Arag{\'o}n-Salamanca}, A. and {De Lucia}, G. and {Moretti}, A. and {Gladders}, M. and {Abramson}, L. and {Halliday}, C.},
        title = "{The galaxy stellar mass function and its evolution with time show no dependence on global environment}",
      journal = {\aap},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: clusters: general, galaxies: luminosity function, mass function, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = feb,
       volume = {550},
          eid = {A58},
        pages = {A58},
          doi = {10.1051/0004-6361/201118388},
archivePrefix = {arXiv},
       eprint = {1111.0830},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013A&A...550A..58V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Drory2009,
       author = {{Drory}, N. and {Bundy}, K. and {Leauthaud}, A. and {Scoville}, N. and {Capak}, P. and {Ilbert}, O. and {Kartaltepe}, J.~S. and {Kneib}, J.~P. and {McCracken}, H.~J. and {Salvato}, M. and {Sanders}, D.~B. and {Thompson}, D. and {Willott}, C.~J.},
        title = "{The Bimodal Galaxy Stellar Mass Function in the COSMOS Survey to z \raisebox{-0.5ex}\textasciitilde 1: A Steep Faint End and a New Galaxy Dichotomy}",
      journal = {\apj},
     keywords = {cosmology: observations, galaxies: evolution, galaxies: luminosity function, mass function, surveys, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2009,
        month = dec,
       volume = {707},
       number = {2},
        pages = {1595-1609},
          doi = {10.1088/0004-637X/707/2/1595},
archivePrefix = {arXiv},
       eprint = {0910.5720},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009ApJ...707.1595D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Lustig2022,
       author = {{Lustig}, Peter and {Strazzullo}, Veronica and {Remus}, Rhea-Silvia and {D'Eugenio}, Chiara and {Daddi}, Emanuele and {Burkert}, Andreas and {De Lucia}, Gabriella and {Delvecchio}, Ivan and {Dolag}, Klaus and {Fontanot}, Fabio and {Gobat}, Raphael and {Mohr}, Joseph J. and {Onodera}, Masato and {Pannella}, Maurilio and {Pillepich}, Annalisa and {Renzini}, Alvio},
        title = "{Massive quiescent galaxies at $z\sim3$: a comparison of selection, stellar population and structural properties with simulation predictions}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = jan,
          eid = {arXiv:2201.09068},
        pages = {arXiv:2201.09068},
archivePrefix = {arXiv},
       eprint = {2201.09068},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220109068L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{James1975,
       author = {{James}, F. and {Roos}, M.},
        title = "{Minuit - a system for function minimization and analysis of the parameter errors and correlations}",
      journal = {Computer Physics Communications},
         year = 1975,
        month = dec,
       volume = {10},
       number = {6},
        pages = {343-367},
          doi = {10.1016/0010-4655(75)90039-9},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1975CoPhC..10..343J},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{emcee,
   author = {{Foreman-Mackey}, D. and {Hogg}, D.~W. and {Lang}, D. and {Goodman}, J.},
    title = {emcee: The MCMC Hammer},
  journal = {PASP},
     year = 2013,
   volume = 125,
    pages = {306-312},
   eprint = {1202.3665},
      doi = {10.1086/670067}
}

@ARTICLE{Goodman2010,
       author = {{Goodman}, Jonathan and {Weare}, Jonathan},
        title = "{Ensemble samplers with affine invariance}",
      journal = {Communications in Applied Mathematics and Computational Science},
     keywords = {Markov chain Monte Carlo, affine invariance, ensemble samplers},
         year = 2010,
        month = jan,
       volume = {5},
       number = {1},
        pages = {65-80},
          doi = {10.2140/camcos.2010.5.65},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010CAMCS...5...65G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Hogg2010,
       author = {{Hogg}, David W. and {Bovy}, Jo and {Lang}, Dustin},
        title = "{Data analysis recipes: Fitting a model to data}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Data Analysis, Statistics and Probability},
         year = 2010,
        month = aug,
          eid = {arXiv:1008.4686},
        pages = {arXiv:1008.4686},
archivePrefix = {arXiv},
       eprint = {1008.4686},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010arXiv1008.4686H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Straatman2015,
       author = {{Straatman}, Caroline M.~S. and {Labb{\'e}}, Ivo and {Spitler}, Lee R. and {Glazebrook}, Karl and {Tomczak}, Adam and {Allen}, Rebecca and {Brammer}, Gabriel B. and {Cowley}, Michael and {van Dokkum}, Pieter and {Kacprzak}, Glenn G. and {Kawinwanichakij}, Lalit and {Mehrtens}, Nicola and {Nanayakkara}, Themiya and {Papovich}, Casey and {Persson}, S. Eric and {Quadri}, Ryan F. and {Rees}, Glen and {Tilvi}, Vithal and {Tran}, Kim-Vy H. and {Whitaker}, Katherine E.},
        title = "{The Sizes of Massive Quiescent and Star-forming Galaxies at z {\ensuremath{\sim}} 4 with ZFOURGE and CANDELS}",
      journal = {\apjl},
     keywords = {cosmology: observations, galaxies: evolution, galaxies: formation, galaxies: high-redshift, infrared: galaxies, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2015,
        month = jul,
       volume = {808},
       number = {1},
          eid = {L29},
        pages = {L29},
          doi = {10.1088/2041-8205/808/1/L29},
archivePrefix = {arXiv},
       eprint = {1506.01380},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015ApJ...808L..29S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Mawatari2020,
       author = {{Mawatari}, Ken and {Inoue}, Akio K. and {Hashimoto}, Takuya and {Silverman}, John and {Kajisawa}, Masaru and {Yamanaka}, Satoshi and {Yamada}, Toru and {Davidzon}, Iary and {Capak}, Peter and {Lin}, Lihwai and {Hsieh}, Bau-Ching and {Taniguchi}, Yoshiaki and {Tanaka}, Masayuki and {Ono}, Yoshiaki and {Harikane}, Yuichi and {Sugahara}, Yuma and {Fujimoto}, Seiji and {Nagao}, Tohru},
        title = "{Balmer Break Galaxy Candidates at z {\ensuremath{\sim}} 6: A Potential View on the Star Formation Activity at z {\ensuremath{\gtrsim}} 14}",
      journal = {\apj},
     keywords = {595, 435, 1569, 734, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = feb,
       volume = {889},
       number = {2},
          eid = {137},
        pages = {137},
          doi = {10.3847/1538-4357/ab6596},
archivePrefix = {arXiv},
       eprint = {1912.10954},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...889..137M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Mawatari2016,
       author = {{Mawatari}, Ken and {Yamada}, Toru and {Fazio}, Giovanni G. and {Huang}, Jia-Sheng and {Ashby}, Matthew L.~N.},
        title = "{Possible identification of massive and evolved galaxies at z {\ensuremath{\gtrsim}} 5}",
      journal = {\pasj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = jun,
       volume = {68},
       number = {3},
          eid = {46},
        pages = {46},
          doi = {10.1093/pasj/psw041},
archivePrefix = {arXiv},
       eprint = {1603.08394},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016PASJ...68...46M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Davidzon2018,
       author = {{Davidzon}, Iary and {Ilbert}, Olivier and {Faisst}, Andreas L. and {Sparre}, Martin and {Capak}, Peter L.},
        title = "{An Alternate Approach to Measure Specific Star Formation Rates at 2 z 7}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: high-redshift, galaxies: star formation, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2018,
        month = jan,
       volume = {852},
       number = {2},
          eid = {107},
        pages = {107},
          doi = {10.3847/1538-4357/aaa19e},
archivePrefix = {arXiv},
       eprint = {1712.03959},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ApJ...852..107D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Martis2016,
       author = {{Martis}, Nicholas S. and {Marchesini}, Danilo and {Brammer}, Gabriel B. and {Muzzin}, Adam and {Labb{\'e}}, Ivo and {Momcheva}, Ivelina G. and {Skelton}, Rosalind E. and {Stefanon}, Mauro and {van Dokkum}, Pieter G. and {Whitaker}, Katherine E.},
        title = "{The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z = 3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe}",
      journal = {\apjl},
     keywords = {galaxies: evolution, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = aug,
       volume = {827},
       number = {2},
          eid = {L25},
        pages = {L25},
          doi = {10.3847/2041-8205/827/2/L25},
archivePrefix = {arXiv},
       eprint = {1606.04090},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016ApJ...827L..25M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Brammer2011,
       author = {{Brammer}, Gabriel B. and {Whitaker}, K.~E. and {van Dokkum}, P.~G. and {Marchesini}, D. and {Franx}, M. and {Kriek}, M. and {Labb{\'e}}, I. and {Lee}, K. -S. and {Muzzin}, A. and {Quadri}, R.~F. and {Rudnick}, G. and {Williams}, R.},
        title = "{The Number Density and Mass Density of Star-forming and Quiescent Galaxies at 0.4 <= z <= 2.2}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2011,
        month = sep,
       volume = {739},
       number = {1},
          eid = {24},
        pages = {24},
          doi = {10.1088/0004-637X/739/1/24},
archivePrefix = {arXiv},
       eprint = {1104.2595},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJ...739...24B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Moneti2022,
       author = {{Moneti}, Andrea and {McCracken}, H.~J. and {Shuntov}, M. and {Kauffmann}, O.~B. and {Capak}, P. and {Davidzon}, I. and {Ilbert}, O. and {Scarlata}, C. and {Toft}, S. and {Weaver}, J. and {Chary}, R. and {Cuby}, J. and {Faisst}, A.~L. and {Masters}, D.~C. and {McPartland}, C. and {Mobasher}, B. and {Sanders}, D.~B. and {Scaramella}, R. and {Stern}, D. and {Szapudi}, I. and {Teplitz}, H. and {Zalesky}, L. and {Amara}, A. and {Auricchio}, N. and {Bodendorf}, C. and {Bonino}, D. and {Branchini}, E. and {Brau-Nogue}, S. and {Brescia}, M. and {Brinchmann}, J. and {Capobianco}, V. and {Carbone}, C. and {Carretero}, J. and {Castander}, F.~J. and {Castellano}, M. and {Cavuoti}, S. and {Cimatti}, A. and {Cledassou}, R. and {Congedo}, G. and {Conselice}, C.~J. and {Conversi}, L. and {Copin}, Y. and {Corcione}, L. and {Costille}, A. and {Cropper}, M. and {Da Silva}, A. and {Degaudenzi}, H. and {Douspis}, M. and {Dubath}, F. and {Duncan}, C.~A.~J. and {Dupac}, X. and {Dusini}, S. and {Farrens}, S. and {Ferriol}, S. and {Fosalba}, P. and {Frailis}, M. and {Franceschi}, E. and {Fumana}, M. and {Garilli}, B. and {Gillis}, B. and {Giocoli}, C. and {Granett}, B.~R. and {Grazian}, A. and {Grupp}, F. and {Haugan}, S.~V.~H. and {Hoekstra}, H. and {Holmes}, W. and {Hormuth}, F. and {Hudelot}, P. and {Jahnke}, K. and {Kermiche}, S. and {Kiessling}, A. and {Kilbinger}, M. and {Kitching}, T. and {Kohley}, R. and {Kuemmel}, M. and {Kunz}, M. and {Kurki-Suonio}, H. and {Ligori}, S. and {Lilje}, P.~B. and {Lloro}, I. and {Maiorano}, E. and {Mansutti}, O. and {Marggraf}, O. and {Markovic}, K. and {Marulli}, F. and {Massey}, R. and {Maurogordato}, S. and {Meneghetti}, M. and {Merlin}, E. and {Meylan}, G. and {Moresco}, M. and {Moscardini}, L. and {Munari}, E. and {Niemi}, S.~M. and {Padilla}, C. and {Paltani}, S. and {Pasian}, F. and {Pedersen}, K. and {Pires}, S. and {Poncet}, M. and {Popa}, L. and {Pozzetti}, L. and {Raison}, F. and {Rebolo}, R. and {Rhodes}, J. and {Rix}, H. and {Roncarelli}, M. and {Rossetti}, E. and {Saglia}, R. and {Schneider}, P. and {Secroun}, A. and {Seidel}, G. and {Serrano}, S. and {Sirignano}, C. and {Sirri}, G. and {Stanco}, L. and {Tallada-Crespi}, P. and {Taylor}, A.~N. and {Tereno}, I. and {Toledo-Moreo}, R. and {Torradeflot}, F. and {Wang}, Y. and {Welikala}, N. and {Weller}, J. and {Zamorani}, G. and {Zoubian}, J. and {Andreon}, S. and {Bardelli}, S. and {Camera}, S. and {Gracia-Carpio}, J. and {Medinaceli}, E. and {Mei}, S. and {Polenta}, G. and {Romelli}, E. and {Sureau}, F. and {Tenti}, M. and {Vassallo}, T. and {Zacchei}, A. and {Zucca}, E. and {Baccigalupi}, C. and {Balaguera-Antolinez}, A. and {Bernardeau}, F. and {Biviano}, A. and {Bolzonella}, M. and {Bozzo}, E. and {Burigana}, C. and {Cabanac}, R. and {Cappi}, A. and {Carvalho}, C.~S. and {Casas}, S. and {Castignani}, G. and {Colodro-Conde}, C. and {Coupon}, J. and {Courtois}, H.~M. and {Di Ferdinando}, D. and {Farina}, M. and {Finelli}, F. and {Flose-Reimberg}, P. and {Fotopoulou}, S. and {Galeotta}, S. and {Ganga}, K. and {Garcia-Bellido}, J. and {Gaztanaga}, E. and {Gozaliasl}, G. and {Hook}, I. and {Joachimi}, B. and {Kansal}, V. and {Keihanen}, E. and {Kirkpatrick}, C.~C. and {Lindholm}, V. and {Mainetti}, G. and {Maino}, D. and {Maoli}, R. and {Martinelli}, M. and {Martinet}, N. and {Maturi}, M. and {Metcalf}, R.~B. and {Morgante}, G. and {Morisset}, N. and {Nucita}, A. and {Patrizii}, L. and {Potter}, D. and {Renzi}, A. and {Riccio}, G. and {Sanchez}, A.~G. and {Sapone}, D. and {Schirmer}, M. and {Schultheis}, M. and {Scottez}, V. and {Sefusatti}, E. and {Teyssier}, R. and {Tubio}, O. and {Tutusaus}, I. and {Valiviita}, J. and {Viel}, M. and {Hildebrandt}, H.},
        title = "{Euclid preparation: XVIII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fields}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2021,
        month = oct,
          eid = {arXiv:2110.13928},
        pages = {arXiv:2110.13928},
archivePrefix = {arXiv},
       eprint = {2110.13928},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv211013928M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Casey2021,
       author = {{Casey}, Caitlin M. and {Zavala}, Jorge A. and {Manning}, Sinclaire M. and {Aravena}, Manuel and {B{\'e}thermin}, Matthieu and {Caputi}, Karina I. and {Champagne}, Jaclyn B. and {Clements}, David L. and {Drew}, Patrick and {Finkelstein}, Steven L. and {Fujimoto}, Seiji and {Hayward}, Christopher C. and {Dekel}, Anton M. and {Kokorev}, Vasily and {Lagos}, Claudia del P. and {Long}, Arianna S. and {Magdis}, Georgios E. and {Man}, Allison W.~S. and {Mitsuhashi}, Ikki and {Popping}, Gerg{\"o} and {Spilker}, Justin and {Staguhn}, Johannes and {Talia}, Margherita and {Toft}, Sune and {Treister}, Ezequiel and {Weaver}, John R. and {Yun}, Min},
        title = "{Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies}",
      journal = {\apj},
     keywords = {1061, 1647, 412, 734, 17, 790, 1570, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2021,
        month = dec,
       volume = {923},
       number = {2},
          eid = {215},
        pages = {215},
          doi = {10.3847/1538-4357/ac2eb4},
archivePrefix = {arXiv},
       eprint = {2110.06930},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...923..215C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Jin2019,
       author = {{Jin}, S. and {Daddi}, E. and {Magdis}, G.~E. and {Liu}, D. and {Schinnerer}, E. and {Papadopoulos}, P.~P. and {Gu}, Q. and {Gao}, Y. and {Calabr{\`o}}, A.},
        title = "{Discovery of Four Apparently Cold Dusty Galaxies at z = 3.62-5.85 in the COSMOS Field: Direct Evidence of Cosmic Microwave Background Impact on High-redshift Galaxy Observables}",
      journal = {\apj},
     keywords = {Dust continuum emission, Far infrared astronomy, Starburst galaxies, Luminous infrared galaxies, Submillimeter astronomy, High-redshift galaxies, Cosmic microwave background radiation, Interstellar medium, Galaxy evolution, Galaxy formation, 412, 529, 1570, 946, 1647, 734, 322, 847, 594, 595, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2019,
        month = dec,
       volume = {887},
       number = {2},
          eid = {144},
        pages = {144},
          doi = {10.3847/1538-4357/ab55d6},
archivePrefix = {arXiv},
       eprint = {1906.00040},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...887..144J},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{Bertin2010,
       author = {{Bertin}, Emmanuel},
        title = "{SWarp: Resampling and Co-adding FITS Images Together}",
     keywords = {Software},
         year = 2010,
        month = oct,
          eid = {ascl:1010.068},
        pages = {ascl:1010.068},
archivePrefix = {ascl},
       eprint = {1010.068},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010ascl.soft10068B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Gabor2015,
       author = {{Gabor}, J.~M. and {Dav{\'e}}, R.},
        title = "{Hot gas in massive haloes drives both mass quenching and environment quenching}",
      journal = {\mnras},
     keywords = {galaxies: clusters: general, galaxies: evolution, galaxies: formation, galaxies: groups: general, galaxies: haloes, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2015,
        month = feb,
       volume = {447},
       number = {1},
        pages = {374-391},
          doi = {10.1093/mnras/stu2399},
archivePrefix = {arXiv},
       eprint = {1405.1043},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015MNRAS.447..374G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{Kartaltepe_COSMOSWeb,
       author = {{Kartaltepe}, Jeyhan and {Casey}, Caitlin M. and {Bagley}, Micaela and {Bongiorno}, Angela and {Capak}, Peter Lawrence and {Champagne}, Jaclyn and {Cooke}, Kevin C. and {Cooper}, Olivia and {Darvish}, Behnam and {Davidzon}, Iary and {Drakos}, Nicole and {Drew}, Patrick and {Faisst}, Andreas L. and {Finkelstein}, Steven L. and {Hayward}, Christopher and {Hemmati}, Shoubaneh and {Hirschmann}, Michaela and {Ilbert}, Olivier and {Jahnke}, Knud and {Koekemoer}, Anton M. and {Liu}, Daizhong and {Long}, Arianna and {Magdis}, Georgios and {Manning}, Sinclaire and {Maraston}, Claudia and {Martin}, Crystal Linn and {Massey}, Richard J. and {McCleary}, Jacqueline and {McCracken}, Henry Joy and {Nayyeri}, Hooshang and {Renzini}, Alvio and {Rhodes}, Jason D. and {Rich}, R. Michael and {Robertson}, Brant and {Rose}, Caitlin and {Sanders}, David B. and {Scarlata}, Claudia and {Scoville}, Nicholas Z. and {Sheth}, Kartik and {Silverman}, John David and {Sparre}, Martin and {Talia}, Margherita and {Toft}, Sune and {Trakhtenbrot}, Benny and {Vanderhoof}, Brittany and {Vardoulaki}, Eleni and {Whitaker}, Katherine E. and {Wilkins}, Stephen Matthew and {Zavala}, Jorge},
        title = "{COSMOS-Webb: The Webb Cosmic Origins Survey}",
 howpublished = {JWST Proposal. Cycle 1},
         year = 2021,
        month = mar,
        pages = {1727},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021jwst.prop.1727K},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{Ferruit_JADES,
       author = {{Ferruit}, Pierre},
        title = "{NIRCam-NIRSpec galaxy assembly survey - GOODS-S - part \#1b}",
 howpublished = {JWST Proposal. Cycle 1},
         year = 2017,
        month = jul,
        pages = {1210},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017jwst.prop.1210F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{Eisenstein_JADES,
       author = {{Eisenstein}, Daniel J. and {Ferruit}, Pierre and {Rieke}, Marcia J.},
        title = "{NIRCam-NIRSpec galaxy assembly survey - GOODS-N}",
 howpublished = {JWST Proposal. Cycle 1},
         year = 2017,
        month = jun,
        pages = {1181},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017jwst.prop.1181E},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@MISC{Finkelstein_CEERS,
       author = {{Finkelstein}, Steven L. and {Dickinson}, Mark and {Ferguson}, Harry C. and {Grazian}, Andrea and {Grogin}, Norman and {Kartaltepe}, Jeyhan and {Kewley}, Lisa and {Kocevski}, Dale D. and {Koekemoer}, Anton M. and {Lotz}, Jennifer and {Papovich}, Casey and {Pentericci}, Laura and {Perez-Gonzalez}, Pablo G. and {Pirzkal}, Norbert and {Ravindranath}, Swara and {Somerville}, Rachel S. and {Trump}, Jonathan R. and {Wilkins}, Stephen Matthew},
        title = "{The Cosmic Evolution Early Release Science (CEERS) Survey}",
 howpublished = {JWST Proposal ID 1345. Cycle 0 Early Release Science},
         year = 2017,
        month = nov,
        pages = {1345},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017jwst.prop.1345F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{Finkelstein_WDEEP,
       author = {{Finkelstein}, Steven L. and {Papovich}, Casey and {Pirzkal}, Norbert and {Bagley}, Micaela and {Berg}, Danielle and {Castellano}, Marco and {Chavez Ortiz}, Oscar Antonio and {Chworowsky}, Katherine and {Dave}, Romeel and {Dickinson}, Mark and {Estrada-Carpenter}, Vicente and {Faber}, Sandra M. and {Ferguson}, Harry C. and {Fontana}, Adriano and {Giavalisco}, Mauro and {Grazian}, Andrea and {Grogin}, Norman and {Jaskot}, Anne and {Jung}, Intae and {Kartaltepe}, Jeyhan and {Kewley}, Lisa and {Kirkpatrick}, Allison and {Kocevski}, Dale D. and {Larson}, Rebecca L. and {Leung}, Gene C.~K. and {Lotz}, Jennifer and {Mantha}, Kameswara Bharadwaj and {Matharu}, Jasleen and {McCarron}, Adam and {McIntosh}, Daniel and {Natarajan}, Priya and {Pentericci}, Laura and {Ravindranath}, Swara and {Rodriguez-Gomez}, Vicente and {Rothberg}, Barry and {Ryan}, Russell E. and {Simons}, Raymond and {Snyder}, Greg and {Somerville}, Rachel S. and {Trump}, Jonathan R. and {Wilkins}, Stephen Matthew and {Yung}, L.~Y. Aaron},
        title = "{The Webb Deep Extragalactic Exploratory Public (WDEEP) Survey: Feedback in Low-Mass Galaxies from Cosmic Dawn to Dusk}",
 howpublished = {JWST Proposal. Cycle 1},
         year = 2021,
        month = mar,
        pages = {2079},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021jwst.prop.2079F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{Labbe_UNCOVER,
       author = {{Labbe}, Ivo and {Bezanson}, Rachel and {Atek}, Hakim and {Brammer}, Gabriel and {Coe}, Dan and {Dayal}, Pratika and {Feldmann}, Robert and {Forster Schreiber}, N.~M. and {Franx}, Marijn and {Geha}, Marla C. and {Glazebrook}, Karl and {Greene}, Jenny Emma and {Juneau}, Stephanie and {Kassin}, Susan and {Kriek}, Mariska and {Leja}, Joel and {Marchesini}, Danilo and {Maseda}, Michael and {Mowla}, Lamiya and {Muzzin}, Adam and {Nanayakkara}, Themiya and {Nelson}, Erica and {Oesch}, Pascal and {Pacifici}, Camilla and {Papovich}, Casey and {Price}, Sedona H. and {Shapley}, Alice E. and {Stefanon}, Mauro and {Taylor}, Edward N. and {Whitaker}, Katherine E. and {Williams}, Christina C. and {Zitrin}, Adi and {de Graaff}, Anna G. and {van Dokkum}, Pieter},
        title = "{UNCOVER: Ultra-deep NIRCam and NIRSpec Observations Before the Epoch of Reionization}",
 howpublished = {JWST Proposal. Cycle 1},
         year = 2021,
        month = mar,
        pages = {2561},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021jwst.prop.2561L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Schenker2013,
       author = {{Schenker}, Matthew A. and {Robertson}, Brant E. and {Ellis}, Richard S. and {Ono}, Yoshiaki and {McLure}, Ross J. and {Dunlop}, James S. and {Koekemoer}, Anton and {Bowler}, Rebecca A.~A. and {Ouchi}, Masami and {Curtis-Lake}, Emma and {Rogers}, Alexander B. and {Schneider}, Evan and {Charlot}, Stephane and {Stark}, Daniel P. and {Furlanetto}, Steven R. and {Cirasuolo}, Michele},
        title = "{The UV Luminosity Function of Star-forming Galaxies via Dropout Selection at Redshifts z \raisebox{-0.5ex}\textasciitilde 7 and 8 from the 2012 Ultra Deep Field Campaign}",
      journal = {\apj},
     keywords = {dark ages, reionization, first stars, galaxies: evolution, galaxies: formation, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = may,
       volume = {768},
       number = {2},
          eid = {196},
        pages = {196},
          doi = {10.1088/0004-637X/768/2/196},
archivePrefix = {arXiv},
       eprint = {1212.4819},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJ...768..196S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Bouwens2012a,
       author = {{Bouwens}, R.~J. and {Illingworth}, G.~D. and {Oesch}, P.~A. and {Franx}, M. and {Labb{\'e}}, I. and {Trenti}, M. and {van Dokkum}, P. and {Carollo}, C.~M. and {Gonz{\'a}lez}, V. and {Smit}, R. and {Magee}, D.},
        title = "{UV-continuum Slopes at z \raisebox{-0.5ex}\textasciitilde 4-7 from the HUDF09+ERS+CANDELS Observations: Discovery of a Well-defined UV Color-Magnitude Relationship for z >= 4 Star-forming Galaxies}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2012,
        month = aug,
       volume = {754},
       number = {2},
          eid = {83},
        pages = {83},
          doi = {10.1088/0004-637X/754/2/83},
archivePrefix = {arXiv},
       eprint = {1109.0994},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012ApJ...754...83B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Bouwens2012b,
       author = {{Bouwens}, R.~J. and {Illingworth}, G.~D. and {Oesch}, P.~A. and {Trenti}, M. and {Labb{\'e}}, I. and {Franx}, M. and {Stiavelli}, M. and {Carollo}, C.~M. and {van Dokkum}, P. and {Magee}, D.},
        title = "{Lower-luminosity Galaxies Could Reionize the Universe: Very Steep Faint-end Slopes to the UV Luminosity Functions at z >= 5-8 from the HUDF09 WFC3/IR Observations}",
      journal = {\apjl},
     keywords = {galaxies: evolution, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2012,
        month = jun,
       volume = {752},
       number = {1},
          eid = {L5},
        pages = {L5},
          doi = {10.1088/2041-8205/752/1/L5},
archivePrefix = {arXiv},
       eprint = {1105.2038},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012ApJ...752L...5B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Carnall_2018,
       author = {{Carnall}, A.~C. and {McLure}, R.~J. and {Dunlop}, J.~S. and {Dav{\'e}}, R.},
        title = "{Inferring the star formation histories of massive quiescent galaxies with BAGPIPES: evidence for multiple quenching mechanisms}",
      journal = {\mnras},
     keywords = {methods: statistical, galaxies: evolution, galaxies: star formation, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2018,
        month = nov,
       volume = {480},
       number = {4},
        pages = {4379-4401},
          doi = {10.1093/mnras/sty2169},
archivePrefix = {arXiv},
       eprint = {1712.04452},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.4379C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Vijayan2021_FLARES,
       author = {{Vijayan}, Aswin P. and {Lovell}, Christopher C. and {Wilkins}, Stephen M. and {Thomas}, Peter A. and {Barnes}, David J. and {Irodotou}, Dimitrios and {Kuusisto}, Jussi and {Roper}, William J.},
        title = "{First Light And Reionization Epoch Simulations (FLARES) - II: The photometric properties of high-redshift galaxies}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: general, galaxies: high-redshift, galaxies: photometry, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = mar,
       volume = {501},
       number = {3},
        pages = {3289-3308},
          doi = {10.1093/mnras/staa3715},
archivePrefix = {arXiv},
       eprint = {2008.06057},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.501.3289V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Lovell2021_FLARES,
       author = {{Lovell}, Christopher C. and {Vijayan}, Aswin P. and {Thomas}, Peter A. and {Wilkins}, Stephen M. and {Barnes}, David J. and {Irodotou}, Dimitrios and {Roper}, Will},
        title = "{First Light And Reionization Epoch Simulations (FLARES) - I. Environmental dependence of high-redshift galaxy evolution}",
      journal = {\mnras},
     keywords = {galaxies: abundances, galaxies: evolution, galaxies: high-redshift, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = jan,
       volume = {500},
       number = {2},
        pages = {2127-2145},
          doi = {10.1093/mnras/staa3360},
archivePrefix = {arXiv},
       eprint = {2004.07283},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.500.2127L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Brinchmann2004,
       author = {{Brinchmann}, J. and {Charlot}, S. and {White}, S.~D.~M. and {Tremonti}, C. and {Kauffmann}, G. and {Heckman}, T. and {Brinkmann}, J.},
        title = "{The physical properties of star-forming galaxies in the low-redshift Universe}",
      journal = {\mnras},
     keywords = {surveys, galaxies: abundances, galaxies: evolution, galaxies: fundamental parameters, galaxies: general, Astrophysics},
         year = 2004,
        month = jul,
       volume = {351},
       number = {4},
        pages = {1151-1179},
          doi = {10.1111/j.1365-2966.2004.07881.x},
archivePrefix = {arXiv},
       eprint = {astro-ph/0311060},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2004MNRAS.351.1151B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Noeske2007,
       author = {{Noeske}, K.~G. and {Weiner}, B.~J. and {Faber}, S.~M. and {Papovich}, C. and {Koo}, D.~C. and {Somerville}, R.~S. and {Bundy}, K. and {Conselice}, C.~J. and {Newman}, J.~A. and {Schiminovich}, D. and {Le Floc'h}, E. and {Coil}, A.~L. and {Rieke}, G.~H. and {Lotz}, J.~M. and {Primack}, J.~R. and {Barmby}, P. and {Cooper}, M.~C. and {Davis}, M. and {Ellis}, R.~S. and {Fazio}, G.~G. and {Guhathakurta}, P. and {Huang}, J. and {Kassin}, S.~A. and {Martin}, D.~C. and {Phillips}, A.~C. and {Rich}, R.~M. and {Small}, T.~A. and {Willmer}, C.~N.~A. and {Wilson}, G.},
        title = "{Star Formation in AEGIS Field Galaxies since z=1.1: The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-forming Galaxies}",
      journal = {\apjl},
     keywords = {Galaxies: Evolution, Galaxies: Formation, Galaxies: High-Redshift, Galaxies: Starburst, Astrophysics},
         year = 2007,
        month = may,
       volume = {660},
       number = {1},
        pages = {L43-L46},
          doi = {10.1086/517926},
archivePrefix = {arXiv},
       eprint = {astro-ph/0701924},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007ApJ...660L..43N},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2007ApJ...670..156D,
       author = {{Daddi}, E. and {Dickinson}, M. and {Morrison}, G. and {Chary}, R. and {Cimatti}, A. and {Elbaz}, D. and {Frayer}, D. and {Renzini}, A. and {Pope}, A. and {Alexander}, D.~M. and {Bauer}, F.~E. and {Giavalisco}, M. and {Huynh}, M. and {Kurk}, J. and {Mignoli}, M.},
        title = "{Multiwavelength Study of Massive Galaxies at z\raisebox{-0.5ex}\textasciitilde2. I. Star Formation and Galaxy Growth}",
      journal = {\apj},
     keywords = {Cosmology: Observations, Galaxies: Evolution, Galaxies: Formation, Galaxies: High-Redshift, Galaxies: Starburst, Astrophysics},
         year = 2007,
        month = nov,
       volume = {670},
       number = {1},
        pages = {156-172},
          doi = {10.1086/521818},
archivePrefix = {arXiv},
       eprint = {0705.2831},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007ApJ...670..156D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Daddi2007,
       author = {{Daddi}, E. and {Dickinson}, M. and {Morrison}, G. and {Chary}, R. and {Cimatti}, A. and {Elbaz}, D. and {Frayer}, D. and {Renzini}, A. and {Pope}, A. and {Alexander}, D.~M. and {Bauer}, F.~E. and {Giavalisco}, M. and {Huynh}, M. and {Kurk}, J. and {Mignoli}, M.},
        title = "{Multiwavelength Study of Massive Galaxies at z\raisebox{-0.5ex}\textasciitilde2. I. Star Formation and Galaxy Growth}",
      journal = {\apj},
     keywords = {Cosmology: Observations, Galaxies: Evolution, Galaxies: Formation, Galaxies: High-Redshift, Galaxies: Starburst, Astrophysics},
         year = 2007,
        month = nov,
       volume = {670},
       number = {1},
        pages = {156-172},
          doi = {10.1086/521818},
archivePrefix = {arXiv},
       eprint = {0705.2831},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007ApJ...670..156D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Whitaker2012,
       author = {{Whitaker}, Katherine E. and {van Dokkum}, Pieter G. and {Brammer}, Gabriel and {Franx}, Marijn},
        title = "{The Star Formation Mass Sequence Out to z = 2.5}",
      journal = {\apjl},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2012,
        month = aug,
       volume = {754},
       number = {2},
          eid = {L29},
        pages = {L29},
          doi = {10.1088/2041-8205/754/2/L29},
archivePrefix = {arXiv},
       eprint = {1205.0547},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012ApJ...754L..29W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Whitaker2014,
       author = {{Whitaker}, Katherine E. and {Franx}, Marijn and {Leja}, Joel and {van Dokkum}, Pieter G. and {Henry}, Alaina and {Skelton}, Rosalind E. and {Fumagalli}, Mattia and {Momcheva}, Ivelina G. and {Brammer}, Gabriel B. and {Labb{\'e}}, Ivo and {Nelson}, Erica J. and {Rigby}, Jane R.},
        title = "{Constraining the Low-mass Slope of the Star Formation Sequence at 0.5 < z < 2.5}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Astrophysics of Galaxies},
         year = 2014,
        month = nov,
       volume = {795},
       number = {2},
          eid = {104},
        pages = {104},
          doi = {10.1088/0004-637X/795/2/104},
archivePrefix = {arXiv},
       eprint = {1407.1843},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014ApJ...795..104W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Vijayan2022_FLARES,
       author = {{Vijayan}, Aswin P. and {Wilkins}, Stephen M. and {Lovell}, Christopher C. and {Thomas}, Peter A. and {Camps}, Peter and {Baes}, Maarten and {Trayford}, James and {Kuusisto}, Jussi and {Roper}, William J.},
        title = "{First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn}",
      journal = {\mnras},
     keywords = {methods: numerical, galaxies: formation, galaxies: evolution, galaxies: high-redshift, infrared: galaxies, Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = feb,
          doi = {10.1093/mnras/stac338},
archivePrefix = {arXiv},
       eprint = {2108.00830},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022MNRAS.tmp..355V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Diemer2018_COLOSSUS,
       author = {{Diemer}, Benedikt},
        title = "{COLOSSUS: A Python Toolkit for Cosmology, Large-scale Structure, and Dark Matter Halos}",
      journal = {\apjs},
     keywords = {cosmology: theory, methods: numerical, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2018,
        month = dec,
       volume = {239},
       number = {2},
          eid = {35},
        pages = {35},
          doi = {10.3847/1538-4365/aaee8c},
archivePrefix = {arXiv},
       eprint = {1712.04512},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ApJS..239...35D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Wechsler2018_ARAA,
       author = {{Wechsler}, Risa H. and {Tinker}, Jeremy L.},
        title = "{The Connection Between Galaxies and Their Dark Matter Halos}",
      journal = {\araa},
     keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2018,
        month = sep,
       volume = {56},
        pages = {435-487},
          doi = {10.1146/annurev-astro-081817-051756},
archivePrefix = {arXiv},
       eprint = {1804.03097},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018ARA&A..56..435W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{Mandelbaum2006,
	title = {Galaxy halo masses and satellite fractions from galaxy-galaxy lensing in the {Sloan} {Digital} {Sky} {Survey}: stellar mass, luminosity, morphology and environment dependencies},
	volume = {368},
	issn = {0035-8711},
	shorttitle = {Galaxy halo masses and satellite fractions from galaxy-galaxy lensing in the {Sloan} {Digital} {Sky} {Survey}},
	url = {https://ui.adsabs.harvard.edu/abs/2006MNRAS.368..715M},
	doi = {10.1111/j.1365-2966.2006.10156.x},
	urldate = {2021-10-08},
	journal = {\mnras},
	author = {Mandelbaum, Rachel and Seljak, Uroš and Kauffmann, Guinevere and Hirata, Christopher M. and Brinkmann, Jonathan},
	month = may,
	year = {2006},
	keywords = {Astrophysics, galaxies: haloes, galaxies: stellar content, gravitational lensing},
	pages = {715--731},
}

@article{conroy_connecting_2009,
	title = {Connecting {Galaxies}, {Halos}, and {Star} {Formation} {Rates} {Across} {Cosmic} {Time}},
	volume = {696},
	issn = {0004-637X, 1538-4357},
	url = {http://arxiv.org/abs/0805.3346},
	doi = {10.1088/0004-637X/696/1/620},
	number = {1},
	urldate = {2021-09-30},
	journal = {\apj},
	author = {Conroy, Charlie and Wechsler, Risa H.},
	month = may,
	year = {2009},
	note = {arXiv: 0805.3346},
	keywords = {Astrophysics},
	pages = {620--635},
}

@article{behroozi_comprehensive_2010,
	title = {A {Comprehensive} {Analysis} of {Uncertainties} {Affecting} the {Stellar} {Mass} - {Halo} {Mass} {Relation} for 0{\textless}z{\textless}4},
	volume = {717},
	issn = {0004-637X, 1538-4357},
	url = {http://arxiv.org/abs/1001.0015},
	doi = {10.1088/0004-637X/717/1/379},
	number = {1},
	urldate = {2021-07-03},
	journal = {\apj},
	author = {Behroozi, Peter S. and Conroy, Charlie and Wechsler, Risa H.},
	month = jul,
	year = {2010},
	note = {arXiv: 1001.0015},
	keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
	pages = {379--403},
}

@ARTICLE{Birnboim2003,
       author = {{Birnboim}, Yuval and {Dekel}, Avishai},
        title = "{Virial shocks in galactic haloes?}",
      journal = {\mnras},
     keywords = {hydrodynamics, shock waves, cooling flows, galaxies: formation, galaxies: ISM, dark matter, Astrophysics},
         year = 2003,
        month = oct,
       volume = {345},
       number = {1},
        pages = {349-364},
          doi = {10.1046/j.1365-8711.2003.06955.x},
archivePrefix = {arXiv},
       eprint = {astro-ph/0302161},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2003MNRAS.345..349B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Main2017,
       author = {{Main}, R.~A. and {McNamara}, B.~R. and {Nulsen}, P.~E.~J. and {Russell}, H.~R. and {Vantyghem}, A.~N.},
        title = "{A relationship between halo mass, cooling, active galactic nuclei heating and the co-evolution of massive black holes}",
      journal = {\mnras},
     keywords = {accretion, accretion discs, galaxies: active, galaxies: evolution, galaxies: jets, X-rays: galaxies: clusters, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = feb,
       volume = {464},
       number = {4},
        pages = {4360-4382},
          doi = {10.1093/mnras/stw2644},
archivePrefix = {arXiv},
       eprint = {1510.07046},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017MNRAS.464.4360M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Lilly2013,
       author = {{Lilly}, Simon J. and {Carollo}, C. Marcella and {Pipino}, Antonio and {Renzini}, Alvio and {Peng}, Yingjie},
        title = "{Gas Regulation of Galaxies: The Evolution of the Cosmic Specific Star Formation Rate, the Metallicity-Mass-Star-formation Rate Relation, and the Stellar Content of Halos}",
      journal = {\apj},
     keywords = {dark matter, galaxies: abundances, galaxies: evolution, galaxies: halos, galaxies: ISM, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2013,
        month = aug,
       volume = {772},
       number = {2},
          eid = {119},
        pages = {119},
          doi = {10.1088/0004-637X/772/2/119},
archivePrefix = {arXiv},
       eprint = {1303.5059},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJ...772..119L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Neistein2008,
       author = {{Neistein}, Eyal and {Dekel}, Avishai},
        title = "{Merger rates of dark matter haloes}",
      journal = {\mnras},
     keywords = {gravitation, galaxies: formation, galaxies: haloes, cosmology: theory, dark matter, Astrophysics},
         year = 2008,
        month = aug,
       volume = {388},
       number = {4},
        pages = {1792-1802},
          doi = {10.1111/j.1365-2966.2008.13525.x},
archivePrefix = {arXiv},
       eprint = {0802.0198},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2008MNRAS.388.1792N},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Saintonge2013,
       author = {{Saintonge}, Am{\'e}lie and {Lutz}, Dieter and {Genzel}, Reinhard and {Magnelli}, Benjamin and {Nordon}, Raanan and {Tacconi}, Linda J. and {Baker}, Andrew J. and {Bandara}, Kaushala and {Berta}, Stefano and {F{\"o}rster Schreiber}, Natascha M. and {Poglitsch}, Albrecht and {Sturm}, Eckhard and {Wuyts}, Eva and {Wuyts}, Stijn},
        title = "{Validation of the Equilibrium Model for Galaxy Evolution to z \raisebox{-0.5ex}\textasciitilde 3 through Molecular Gas and Dust Observations of Lensed Star-forming Galaxies}",
      journal = {\apj},
     keywords = {dust, extinction, galaxies: evolution, galaxies: high-redshift, infrared: ISM, ISM: molecules, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2013,
        month = nov,
       volume = {778},
       number = {1},
          eid = {2},
        pages = {2},
          doi = {10.1088/0004-637X/778/1/2},
archivePrefix = {arXiv},
       eprint = {1309.3281},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJ...778....2S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Behroozi2013,
       author = {{Behroozi}, Peter S. and {Wechsler}, Risa H. and {Conroy}, Charlie},
        title = "{The Average Star Formation Histories of Galaxies in Dark Matter Halos from z = 0-8}",
      journal = {\apj},
     keywords = {dark matter, galaxies: abundances, galaxies: evolution, methods: numerical, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2013,
        month = jun,
       volume = {770},
       number = {1},
          eid = {57},
        pages = {57},
          doi = {10.1088/0004-637X/770/1/57},
archivePrefix = {arXiv},
       eprint = {1207.6105},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJ...770...57B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Kaviraj2017,
       author = {{Kaviraj}, S. and {Laigle}, C. and {Kimm}, T. and {Devriendt}, J.~E.~G. and {Dubois}, Y. and {Pichon}, C. and {Slyz}, A. and {Chisari}, E. and {Peirani}, S.},
        title = "{The Horizon-AGN simulation: evolution of galaxy properties over cosmic time}",
      journal = {\mnras},
     keywords = {methods: numerical, galaxies: evolution, galaxies: formation, galaxies: high-redshift, cosmology: theory, large-scale structure of Universe, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = jun,
       volume = {467},
       number = {4},
        pages = {4739-4752},
          doi = {10.1093/mnras/stx126},
archivePrefix = {arXiv},
       eprint = {1605.09379},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017MNRAS.467.4739K},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Padovani2015,
       author = {{Padovani}, P. and {Bonzini}, M. and {Kellermann}, K.~I. and {Miller}, N. and {Mainieri}, V. and {Tozzi}, P.},
        title = "{Radio-faint AGN: a tale of two populations}",
      journal = {\mnras},
     keywords = {surveys, galaxies: active, galaxies: evolution, quasars: general, galaxies: starburst, radio continuum: galaxies, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2015,
        month = sep,
       volume = {452},
       number = {2},
        pages = {1263-1279},
          doi = {10.1093/mnras/stv1375},
archivePrefix = {arXiv},
       eprint = {1506.06554},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015MNRAS.452.1263P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Cicone2015,
       author = {{Cicone}, C. and {Maiolino}, R. and {Gallerani}, S. and {Neri}, R. and {Ferrara}, A. and {Sturm}, E. and {Fiore}, F. and {Piconcelli}, E. and {Feruglio}, C.},
        title = "{Very extended cold gas, star formation and outflows in the halo of a bright quasar at z > 6}",
      journal = {\aap},
     keywords = {galaxies: general, galaxies: ISM, galaxies: evolution, galaxies: high-redshift, quasars: general, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2015,
        month = feb,
       volume = {574},
          eid = {A14},
        pages = {A14},
          doi = {10.1051/0004-6361/201424980},
archivePrefix = {arXiv},
       eprint = {1409.4418},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015A&A...574A..14C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Maiolino2012,
       author = {{Maiolino}, R. and {Gallerani}, S. and {Neri}, R. and {Cicone}, C. and {Ferrara}, A. and {Genzel}, R. and {Lutz}, D. and {Sturm}, E. and {Tacconi}, L.~J. and {Walter}, F. and {Feruglio}, C. and {Fiore}, F. and {Piconcelli}, E.},
        title = "{Evidence of strong quasar feedback in the early Universe}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: high-redshift, quasars: general, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2012,
        month = sep,
       volume = {425},
       number = {1},
        pages = {L66-L70},
          doi = {10.1111/j.1745-3933.2012.01303.x},
archivePrefix = {arXiv},
       eprint = {1204.2904},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012MNRAS.425L..66M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Cicone2014,
       author = {{Cicone}, C. and {Maiolino}, R. and {Sturm}, E. and {Graci{\'a}-Carpio}, J. and {Feruglio}, C. and {Neri}, R. and {Aalto}, S. and {Davies}, R. and {Fiore}, F. and {Fischer}, J. and {Garc{\'\i}a-Burillo}, S. and {Gonz{\'a}lez-Alfonso}, E. and {Hailey-Dunsheath}, S. and {Piconcelli}, E. and {Veilleux}, S.},
        title = "{Massive molecular outflows and evidence for AGN feedback from CO observations}",
      journal = {\aap},
     keywords = {galaxies: active, galaxies: evolution, quasars: general, radio lines: ISM, ISM: molecules, galaxies: ISM, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2014,
        month = feb,
       volume = {562},
          eid = {A21},
        pages = {A21},
          doi = {10.1051/0004-6361/201322464},
archivePrefix = {arXiv},
       eprint = {1311.2595},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014A&A...562A..21C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Roos2015,
       author = {{Roos}, Orianne and {Juneau}, St{\'e}phanie and {Bournaud}, Fr{\'e}d{\'e}ric and {Gabor}, Jared M.},
        title = "{Thermal and Radiative Active Galactic Nucleus Feedback have a Limited Impact on Star Formation in High-redshift Galaxies}",
      journal = {\apj},
     keywords = {galaxies: active, galaxies: high-redshift, galaxies: star formation, ISM: clouds, methods: numerical, radiative transfer, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2015,
        month = feb,
       volume = {800},
       number = {1},
          eid = {19},
        pages = {19},
          doi = {10.1088/0004-637X/800/1/19},
archivePrefix = {arXiv},
       eprint = {1405.7971},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2015ApJ...800...19R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Bieri2017,
       author = {{Bieri}, Rebekka and {Dubois}, Yohan and {Rosdahl}, Joakim and {Wagner}, Alexander and {Silk}, Joseph and {Mamon}, Gary A.},
        title = "{Outflows driven by quasars in high-redshift galaxies with radiation hydrodynamics}",
      journal = {\mnras},
     keywords = {methods: numerical, galaxies: active, galaxies: high-redshift, galaxies: ISM, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = jan,
       volume = {464},
       number = {2},
        pages = {1854-1873},
          doi = {10.1093/mnras/stw2380},
archivePrefix = {arXiv},
       eprint = {1606.06281},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017MNRAS.464.1854B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Habouzit2022,
       author = {{Habouzit}, M{\'e}lanie and {Somerville}, Rachel S. and {Li}, Yuan and {Genel}, Shy and {Aird}, James and {Angl{\'e}s-Alc{\'a}zar}, Daniel and {Dav{\'e}}, Romeel and {Georgiev}, Iskren Y. and {McAlpine}, Stuart and {Rosas-Guevara}, Yetli and {Dubois}, Yohan and {Nelson}, Dylan and {Banados}, Eduardo and {Hernquist}, Lars and {Peirani}, S{\'e}bastien and {Vogelsberger}, Mark},
        title = "{Supermassive black holes in cosmological simulations - II: the AGN population and predictions for upcoming X-ray missions}",
      journal = {\mnras},
     keywords = {black hole physics, methods: numerical, galaxies: evolution, galaxies: formation, Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = jan,
       volume = {509},
       number = {2},
        pages = {3015-3042},
          doi = {10.1093/mnras/stab3147},
archivePrefix = {arXiv},
       eprint = {2111.01802},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022MNRAS.509.3015H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Vito2018,
       author = {{Vito}, F. and {Brandt}, W.~N. and {Yang}, G. and {Gilli}, R. and {Luo}, B. and {Vignali}, C. and {Xue}, Y.~Q. and {Comastri}, A. and {Koekemoer}, A.~M. and {Lehmer}, B.~D. and {Liu}, T. and {Paolillo}, M. and {Ranalli}, P. and {Schneider}, D.~P. and {Shemmer}, O. and {Volonteri}, M. and {Wang}, J.},
        title = "{High-redshift AGN in the Chandra Deep Fields: the obscured fraction and space density of the sub-L$_{*}$ population}",
      journal = {\mnras},
     keywords = {methods: data analysis, surveys, galaxies: active, galaxies: evolution, galaxies: high-redshift, X-rays: galaxies, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = jan,
       volume = {473},
       number = {2},
        pages = {2378-2406},
          doi = {10.1093/mnras/stx2486},
archivePrefix = {arXiv},
       eprint = {1709.07892},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.473.2378V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Salim2007,
       author = {{Salim}, Samir and {Rich}, R. Michael and {Charlot}, St{\'e}phane and {Brinchmann}, Jarle and {Johnson}, Benjamin D. and {Schiminovich}, David and {Seibert}, Mark and {Mallery}, Ryan and {Heckman}, Timothy M. and {Forster}, Karl and {Friedman}, Peter G. and {Martin}, D. Christopher and {Morrissey}, Patrick and {Neff}, Susan G. and {Small}, Todd and {Wyder}, Ted K. and {Bianchi}, Luciana and {Donas}, Jos{\'e} and {Lee}, Young-Wook and {Madore}, Barry F. and {Milliard}, Bruno and {Szalay}, Alex S. and {Welsh}, Barry Y. and {Yi}, Sukyoung K.},
        title = "{UV Star Formation Rates in the Local Universe}",
      journal = {\apjs},
     keywords = {Galaxies: Active, Galaxies: Evolution, Galaxies: Fundamental Parameters, Surveys, Ultraviolet: Galaxies, Astrophysics},
         year = 2007,
        month = dec,
       volume = {173},
       number = {2},
        pages = {267-292},
          doi = {10.1086/519218},
archivePrefix = {arXiv},
       eprint = {0704.3611},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2007ApJS..173..267S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Stern2005,
       author = {{Stern}, Daniel and {Eisenhardt}, Peter and {Gorjian}, Varoujan and {Kochanek}, Christopher S. and {Caldwell}, Nelson and {Eisenstein}, Daniel and {Brodwin}, Mark and {Brown}, Michael J.~I. and {Cool}, Richard and {Dey}, Arjun and {Green}, Paul and {Jannuzi}, Buell T. and {Murray}, Stephen S. and {Pahre}, Michael A. and {Willner}, S.~P.},
        title = "{Mid-Infrared Selection of Active Galaxies}",
      journal = {\apj},
     keywords = {Cosmology: Observations, Galaxies: Formation, Astrophysics},
         year = 2005,
        month = sep,
       volume = {631},
       number = {1},
        pages = {163-168},
          doi = {10.1086/432523},
archivePrefix = {arXiv},
       eprint = {astro-ph/0410523},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2005ApJ...631..163S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Donley2012,
       author = {{Donley}, J.~L. and {Koekemoer}, A.~M. and {Brusa}, M. and {Capak}, P. and {Cardamone}, C.~N. and {Civano}, F. and {Ilbert}, O. and {Impey}, C.~D. and {Kartaltepe}, J.~S. and {Miyaji}, T. and {Salvato}, M. and {Sanders}, D.~B. and {Trump}, J.~R. and {Zamorani}, G.},
        title = "{Identifying Luminous Active Galactic Nuclei in Deep Surveys: Revised IRAC Selection Criteria}",
      journal = {\apj},
     keywords = {galaxies: active, infrared: galaxies, X-rays: galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2012,
        month = apr,
       volume = {748},
       number = {2},
          eid = {142},
        pages = {142},
          doi = {10.1088/0004-637X/748/2/142},
archivePrefix = {arXiv},
       eprint = {1201.3899},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012ApJ...748..142D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Gruppioni2020,
       author = {{Gruppioni}, C. and {B{\'e}thermin}, M. and {Loiacono}, F. and {Le F{\`e}vre}, O. and {Capak}, P. and {Cassata}, P. and {Faisst}, A.~L. and {Schaerer}, D. and {Silverman}, J. and {Yan}, L. and {Bardelli}, S. and {Boquien}, M. and {Carraro}, R. and {Cimatti}, A. and {Dessauges-Zavadsky}, M. and {Ginolfi}, M. and {Fujimoto}, S. and {Hathi}, N.~P. and {Jones}, G.~C. and {Khusanova}, Y. and {Koekemoer}, A.~M. and {Lagache}, G. and {Lemaux}, B.~C. and {Oesch}, P.~A. and {Pozzi}, F. and {Riechers}, D.~A. and {Rodighiero}, G. and {Romano}, M. and {Talia}, M. and {Vallini}, L. and {Vergani}, D. and {Zamorani}, G. and {Zucca}, E.},
        title = "{The ALPINE-ALMA [CII] survey. The nature, luminosity function, and star formation history of dusty galaxies up to z ≃ 6}",
      journal = {\aap},
     keywords = {galaxies: evolution, galaxies: high-redshift, galaxies: luminosity function, mass function, cosmology: observations, submillimeter: galaxies, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2020,
        month = nov,
       volume = {643},
          eid = {A8},
        pages = {A8},
          doi = {10.1051/0004-6361/202038487},
archivePrefix = {arXiv},
       eprint = {2006.04974},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...643A...8G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Forrest2020a,
       author = {{Forrest}, Ben and {Annunziatella}, Marianna and {Wilson}, Gillian and {Marchesini}, Danilo and {Muzzin}, Adam and {Cooper}, M.~C. and {Marsan}, Z. Cemile and {McConachie}, Ian and {Chan}, Jeffrey C.~C. and {Gomez}, Percy and {Kado-Fong}, Erin and {L Barbera}, Francesco and {Labb{\'e}}, Ivo and {Lange-Vagle}, Daniel and {Nantais}, Julie and {Nonino}, Mario and {Pe{\~n}a}, Theodore and {Saracco}, Paolo and {Stefanon}, Mauro and {van der Burg}, Remco F.~J.},
        title = "{An Extremely Massive Quiescent Galaxy at z = 3.493: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models}",
      journal = {\apjl},
     keywords = {Extragalactic astronomy, Galaxy evolution, Galaxy formation, High-redshift galaxies, 506, 594, 595, 734, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = feb,
       volume = {890},
       number = {1},
          eid = {L1},
        pages = {L1},
          doi = {10.3847/2041-8213/ab5b9f},
archivePrefix = {arXiv},
       eprint = {1910.10158},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...890L...1F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Fontana2006,
       author = {{Fontana}, A. and {Salimbeni}, S. and {Grazian}, A. and {Giallongo}, E. and {Pentericci}, L. and {Nonino}, M. and {Fontanot}, F. and {Menci}, N. and {Monaco}, P. and {Cristiani}, S. and {Vanzella}, E. and {de Santis}, C. and {Gallozzi}, S.},
        title = "{The Galaxy mass function up to z =4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies}",
      journal = {\aap},
     keywords = {galaxies: distances and redshift, galaxies: evolution, galaxies: high-redshift, galaxies: fundamental parameters, galaxies: luminosity fuction, mass function, Astrophysics},
         year = 2006,
        month = dec,
       volume = {459},
       number = {3},
        pages = {745-757},
          doi = {10.1051/0004-6361:20065475},
archivePrefix = {arXiv},
       eprint = {astro-ph/0609068},
 primaryClass = {astro-ph},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2006A&A...459..745F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Michalowski2012,
       author = {{Micha{\l}owski}, M.~J. and {Dunlop}, J.~S. and {Cirasuolo}, M. and {Hjorth}, J. and {Hayward}, C.~C. and {Watson}, D.},
        title = "{The stellar masses and specific star-formation rates of submillimetre galaxies}",
      journal = {\aap},
     keywords = {galaxies: active, galaxies: evolution, galaxies: high-redshift, galaxies: ISM, galaxies: starburst, submillimeter: galaxies, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2012,
        month = may,
       volume = {541},
          eid = {A85},
        pages = {A85},
          doi = {10.1051/0004-6361/201016308},
archivePrefix = {arXiv},
       eprint = {1108.6058},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012A&A...541A..85M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Michalowski2014,
       author = {{Micha{\l}owski}, Micha{\l} J. and {Hayward}, Christopher C. and {Dunlop}, James S. and {Bruce}, Victoria A. and {Cirasuolo}, Michele and {Cullen}, Fergus and {Hernquist}, Lars},
        title = "{Determining the stellar masses of submillimetre galaxies: the critical importance of star formation histories}",
      journal = {\aap},
     keywords = {galaxies: fundamental parameters, galaxies: high-redshift, galaxies: starburst, galaxies: star formation, galaxies: stellar content, submillimeter: galaxies, Astrophysics - Astrophysics of Galaxies},
         year = 2014,
        month = nov,
       volume = {571},
          eid = {A75},
        pages = {A75},
          doi = {10.1051/0004-6361/201424174},
archivePrefix = {arXiv},
       eprint = {1405.2335},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014A&A...571A..75M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Conselice2022,
       author = {{Conselice}, Christopher J. and {Mundy}, Carl J. and {Ferreira}, Leonardo and {Duncan}, Kenneth},
        title = "{A direct measurement of galaxy major and minor merger rates and stellar mass accretion histories at $z < 3$ using galaxy pairs in the REFINE survey}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = jul,
          eid = {arXiv:2207.03984},
        pages = {arXiv:2207.03984},
archivePrefix = {arXiv},
       eprint = {2207.03984},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220703984C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{DiTeodoro2022,
       author = {{Di Teodoro}, Enrico M. and {Posti}, Lorenzo and {Fall}, S. Michael and {Ogle}, Patrick M. and {Jarrett}, Thomas and {Appleton}, Philip N. and {Cluver}, Michelle E. and {Haynes}, Martha P. and {Lisenfeld}, Ute},
        title = "{Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = jul,
          eid = {arXiv:2207.02906},
        pages = {arXiv:2207.02906},
archivePrefix = {arXiv},
       eprint = {2207.02906},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220702906D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Peng2014,
       author = {{Peng}, Ying-jie and {Lilly}, Simon J. and {Renzini}, Alvio and {Carollo}, Marcella},
        title = "{Mass and Environment as Drivers of Galaxy Evolution. III. The Constancy of the Faint-end Slope and the Merging of Galaxies}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: fundamental parameters, galaxies: luminosity function, mass function, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2014,
        month = aug,
       volume = {790},
       number = {2},
          eid = {95},
        pages = {95},
          doi = {10.1088/0004-637X/790/2/95},
archivePrefix = {arXiv},
       eprint = {1406.7291},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014ApJ...790...95P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Santini2022,
       author = {{Santini}, P. and {Castellano}, M. and {Fontana}, A. and {Fortuni}, F. and {Menci}, N. and {Merlin}, E. and {Pagul}, A. and {Testa}, V. and {Calabr{\`o}}, A. and {Paris}, D. and {Pentericci}, L.},
        title = "{The Stellar Mass Function in CANDELS and Frontier Fields: the build-up of low mass passive galaxies since z\raisebox{-0.5ex}\textasciitilde3}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = sep,
          eid = {arXiv:2209.11250},
        pages = {arXiv:2209.11250},
archivePrefix = {arXiv},
       eprint = {2209.11250},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220911250S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Forrest2020b,
       author = {{Forrest}, Ben and {Marsan}, Z. Cemile and {Annunziatella}, Marianna and {Wilson}, Gillian and {Muzzin}, Adam and {Marchesini}, Danilo and {Cooper}, M.~C. and {Chan}, Jeffrey C.~C. and {McConachie}, Ian and {Gomez}, Percy and {Kado-Fong}, Erin and {La Barbera}, Francesco and {Lange-Vagle}, Daniel and {Nantais}, Julie and {Nonino}, Mario and {Saracco}, Paolo and {Stefanon}, Mauro and {van der Burg}, Remco F.~J.},
        title = "{The Massive Ancient Galaxies at z > 3 NEar-infrared (MAGAZ3NE) Survey: Confirmation of Extremely Rapid Star Formation and Quenching Timescales for Massive Galaxies in the Early Universe}",
      journal = {\apj},
     keywords = {Galaxy evolution, High-redshift galaxies, Quenched galaxies, 594, 734, 2016, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = nov,
       volume = {903},
       number = {1},
          eid = {47},
        pages = {47},
          doi = {10.3847/1538-4357/abb819},
archivePrefix = {arXiv},
       eprint = {2009.07281},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...903...47F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Forrest2022,
       author = {{Forrest}, Ben and {Wilson}, Gillian and {Muzzin}, Adam and {MArchesini}, Danilo and {Cooper}, M.~C. and {Marsan}, Z. Cemile and {Annunziatella}, Marianna and {McConachie}, Ian and {Zaidi}, Kumail and {Gomez}, Percy and {Urbano Stawinski}, Stephanie M. and {Chang}, Wenjun and {de Lucia}, Gabriella and {La Barbera}, Francesco and {Lubin}, Lori and {Nantais}, Julie and {Pe{\~n}a}, Theodore and {Saracco}, Paolo and {Surace}, Jason and {Stefanon}, Mauro},
        title = "{MAGAZ3NE: High Stellar Velocity Dispersions for Ultra-Massive Quiescent Galaxies at $zrsim3$}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = aug,
          eid = {arXiv:2208.04329},
        pages = {arXiv:2208.04329},
archivePrefix = {arXiv},
       eprint = {2208.04329},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220804329F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Faisst2017,
       author = {{Faisst}, A.~L. and {Carollo}, C.~M. and {Capak}, P.~L. and {Tacchella}, S. and {Renzini}, A. and {Ilbert}, O. and {McCracken}, H.~J. and {Scoville}, N.~Z.},
        title = "{Constraints on Quenching of Z {\ensuremath{\lesssim}} 2 Massive Galaxies from the Evolution of the Average Sizes of Star-forming and Quenched Populations in COSMOS}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: fundamental parameters, galaxies: structure, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2017,
        month = apr,
       volume = {839},
       number = {2},
          eid = {71},
        pages = {71},
          doi = {10.3847/1538-4357/aa697a},
archivePrefix = {arXiv},
       eprint = {1703.09234},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017ApJ...839...71F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Richardson2016,
       author = {{Richardson}, Mark L.~A. and {Scannapieco}, Evan and {Devriendt}, Julien and {Slyz}, Adrianne and {Thacker}, Robert J. and {Dubois}, Yohan and {Wurster}, James and {Silk}, Joseph},
        title = "{Comparing Simulations of AGN Feedback}",
      journal = {\apj},
     keywords = {galaxies: active, galaxies: clusters: general, galaxies: evolution, galaxies: halos, methods: numerical, Astrophysics - Astrophysics of Galaxies},
         year = 2016,
        month = jul,
       volume = {825},
       number = {2},
          eid = {83},
        pages = {83},
          doi = {10.3847/0004-637X/825/2/83},
archivePrefix = {arXiv},
       eprint = {1605.03589},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016ApJ...825...83R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Mitchell2020,
       author = {{Mitchell}, Peter D. and {Schaye}, Joop and {Bower}, Richard G. and {Crain}, Robert A.},
        title = "{Galactic outflow rates in the EAGLE simulations}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: haloes, galaxies: stellar content, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = may,
       volume = {494},
       number = {3},
        pages = {3971-3997},
          doi = {10.1093/mnras/staa938},
archivePrefix = {arXiv},
       eprint = {1910.09566},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.494.3971M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Debuhr2012,
       author = {{Debuhr}, Jackson and {Quataert}, Eliot and {Ma}, Chung-Pei},
        title = "{Galaxy-scale outflows driven by active galactic nuclei}",
      journal = {\mnras},
     keywords = {galaxies: active, galaxies: evolution, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2012,
        month = mar,
       volume = {420},
       number = {3},
        pages = {2221-2231},
          doi = {10.1111/j.1365-2966.2011.20187.x},
archivePrefix = {arXiv},
       eprint = {1107.5579},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012MNRAS.420.2221D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Rigby2022,
       author = {{Rigby}, Jane and {Perrin}, Marshall and {McElwain}, Michael and {Kimble}, Randy and {Friedman}, Scott and {Lallo}, Matt and {Doyon}, Ren{\'e} and {Feinberg}, Lee and {Ferruit}, Pierre and {Glasse}, Alistair and {Rieke}, Marcia and {Rieke}, George and {Wright}, Gillian and {Willott}, Chris and {Colon}, Knicole and {Milam}, Stefanie and {Neff}, Susan and {Stark}, Christopher and {Valenti}, Jeff and {Abell}, Jim and {Abney}, Faith and {Abul-Huda}, Yasin and {Acton}, D. Scott and {Adams}, Evan and {Adler}, David and {Aguilar}, Jonathan and {Ahmed}, Nasif and {Albert}, Lo{\"\i}c and {Alberts}, Stacey and {Aldridge}, David and {Allen}, Marsha and {Altenburg}, Martin and {Alvarez Marquez}, Javier and {Alves de Oliveira}, Catarina and {Andersen}, Greg and {Anderson}, Harry and {Anderson}, Sara and {Argyriou}, Ioannis and {Armstrong}, Amber and {Arribas}, Santiago and {Artigau}, Etienne and {Arvai}, Amanda and {Atkinson}, Charles and {Bacon}, Gregory and {Bair}, Thomas and {Banks}, Kimberly and {Barrientes}, Jaclyn and {Barringer}, Bruce and {Bartosik}, Peter and {Bast}, William and {Baudoz}, Pierre and {Beatty}, Thomas and {Bechtold}, Katie and {Beck}, Tracy and {Bergeron}, Eddie and {Bergkoetter}, Matthew and {Bhatawdekar}, Rachana and {Birkmann}, Stephan and {Blazek}, Ronald and {Blome}, Claire and {Boccaletti}, Anthony and {Boeker}, Torsten and {Boia}, John and {Bonaventura}, Nina and {Bond}, Nicholas and {Bosley}, Kari and {Boucarut}, Ray and {Bourque}, Matthew and {Bouwman}, Jeroen and {Bower}, Gary and {Bowers}, Charles and {Boyer}, Martha and {Bradley}, Larry and {Brady}, Greg and {Braun}, Hannah and {Breda}, David and {Bresnahan}, Pamela and {Bright}, Stacey and {Britt}, Christopher and {Bromenschenkel}, Asa and {Brooks}, Brian and {Brooks}, Keira and {Brown}, Bob and {Brown}, Matthew and {Brown}, Patricia and {Bunker}, Andy and {Burger}, Matthew and {Bushouse}, Howard and {Cale}, Steven and {Cameron}, Alex and {Cameron}, Peter and {Canipe}, Alicia and {Caplinger}, James and {Caputo}, Francis and {Cara}, Mihai and {Carey}, Larkin and {Carniani}, Stefano and {Carrasquilla}, Maria and {Carruthers}, Margaret and {Case}, Michael and {Catherine}, Riggs and {Chance}, Don and {Chapman}, George and {Charlot}, St{\'e}phane and {Charlow}, Brian and {Chayer}, Pierre and {Chen}, Bin and {Cherinka}, Brian and {Chichester}, Sarah and {Chilton}, Zack and {Chonis}, Taylor and {Clampin}, Mark and {Clark}, Charles and {Clark}, Kerry and {Coe}, Dan and {Coleman}, Benee and {Comber}, Brian and {Comeau}, Tom and {Connolly}, Dennis and {Cooper}, James and {Cooper}, Rachel and {Coppock}, Eric and {Correnti}, Matteo and {Cossou}, Christophe and {Coulais}, Alain and {Coyle}, Laura and {Cracraft}, Misty and {Curti}, Mirko and {Cuturic}, Steven and {Davis}, Katherine and {Davis}, Michael and {Dean}, Bruce and {DeLisa}, Amy and {deMeester}, Wim and {Dencheva}, Nadia and {Dencheva}, Nadezhda and {DePasquale}, Joseph and {Deschenes}, Jeremy and {Hunor Detre}, {\"O}rs and {Diaz}, Rosa and {Dicken}, Dan and {DiFelice}, Audrey and {Dillman}, Matthew and {Dixon}, William and {Doggett}, Jesse and {Donaldson}, Tom and {Douglas}, Rob and {DuPrie}, Kimberly and {Dupuis}, Jean and {Durning}, John and {Easmin}, Nilufar and {Eck}, Weston and {Edeani}, Chinwe and {Egami}, Eiichi and {Ehrenwinkler}, Ralf and {Eisenhamer}, Jonathan and {Eisenhower}, Michael and {Elie}, Michelle and {Elliott}, James and {Elliott}, Kyle and {Ellis}, Tracy and {Engesser}, Michael and {Espinoza}, Nestor and {Etienne}, Odessa and {Etxaluze}, Mireya and {Falini}, Patrick and {Feeney}, Matthew and {Ferry}, Malcolm and {Filippazzo}, Joseph and {Fincham}, Brian and {Fix}, Mees and {Flagey}, Nicolas and {Florian}, Michael and {Flynn}, Jim and {Fontanella}, Erin and {Ford}, Terrance and {Forshay}, Peter and {Fox}, Ori and {Franz}, David and {Fu}, Henry and {Fullerton}, Alexander and {Galkin}, Sergey and {Galyer}, Anthony and {Garcia Marin}, Macarena and {Gardner}, Jonathan and {Gardner}, Lisa and {Garland}, Dennis and {Garrett}, Bruce and {Gasman}, Danny and {Gaspar}, Andras and {Gaudreau}, Daniel and {Gauthier}, Peter and {Geers}, Vincent and {Geithner}, Paul and {Gennaro}, Mario and {Giardino}, Giovanna and {Girard}, Julien and {Giuliano}, Mark and {Glassmire}, Kirk and {Glauser}, Adrian and {Glazer}, Stuart and {Godfrey}, John and {Golimowski}, David and {Gollnitz}, David and {Gong}, Fan and {Gonzaga}, Shireen and {Gordon}, Michael and {Gordon}, Karl and {Goudfrooij}, Paul and {Greene}, Thomas and {Greenhouse}, Matthew and {Grimaldi}, Stefano and {Groebner}, Andrew and {Grundy}, Timothy and {Guillard}, Pierre and {Gutman}, Irvin and {Ha}, Kong Q. and {Haderlein}, Peter and {Hagedorn}, Andria and {Hainline}, Kevin and {Haley}, Craig and {Hami}, Maryam and {Hamilton}, Forrest and {Hammel}, Heidi and {Hansen}, Carl and {Harkins}, Tom and {Harr}, Michael and {Hart}, Jessica and {Hart}, Quyen and {Hartig}, George and {Hashimoto}, Ryan and {Haskins}, Sujee and {Hathaway}, William and {Havey}, Keith and {Hayden}, Brian and {Hecht}, Karen and {Heller-Boyer}, Chris and {Henriques}, Caroline and {Henry}, Alaina and {Hermann}, Karl and {Hernandez}, Scarlin and {Hesman}, Brigette and {Hicks}, Brian and {Hilbert}, Bryan and {Hines}, Dean and {Hoffman}, Melissa and {Holfeltz}, Sherie and {Holler}, Bryan J. and {Hoppa}, Jennifer and {Hott}, Kyle and {Howard}, Joseph and {Howard}, Rick and {Hunter}, Alexander and {Hunter}, David and {Hurst}, Brendan and {Husemann}, Bernd and {Hustak}, Leah and {Ilinca Ignat}, Luminita and {Illingworth}, Garth and {Irish}, Sandra and {Jackson}, Wallace and {Jahromi}, Amir and {Jakobsen}, Peter and {James}, LeAndrea and {James}, Bryan and {Januszewski}, William and {Jenkins}, Ann and {Jirdeh}, Hussein and {Johnson}, Phillip and {Johnson}, Timothy and {Jones}, Vicki and {Jones}, Ron and {Jones}, Danny and {Jones}, Olivia and {Jordan}, Ian and {Jordan}, Margaret and {Jurczyk}, Sarah and {Jurling}, Alden and {Kaleida}, Catherine and {Kalmanson}, Phillip and {Kammerer}, Jens and {Kang}, Huijo and {Kao}, Shaw-Hong and {Karakla}, Diane and {Kavanagh}, Patrick and {Kelly}, Doug and {Kendrew}, Sarah and {Kennedy}, Herbert and {Kenny}, Deborah and {Keski-kuha}, Ritva and {Keyes}, Charles and {Kidwell}, Richard and {Kinzel}, Wayne and {Kirk}, Jeff and {Kirkpatrick}, Mark and {Kirshenblat}, Danielle and {Klaassen}, Pamela and {Knapp}, Bryan and {Knight}, J. Scott and {Knollenberg}, Perry and {Koehler}, Robert and {Koekemoer}, Anton and {Kovacs}, Aiden and {Kulp}, Trey and {Kumari}, Nimisha and {Kyprianou}, Mark and {La Massa}, Stephanie and {Labador}, Aurora and {Labiano Ortega}, Alvaro and {Lagage}, Pierre-Olivier and {Lajoie}, Charles-Phillipe and {Lallo}, Matthew and {Lam}, May and {Lamb}, Tracy and {Lambros}, Scott and {Lampenfield}, Richard and {Langston}, James and {Larson}, Kirsten and {Law}, David and {Lawrence}, Jon and {Lee}, David and {Leisenring}, Jarron and {Lepo}, Kelly and {Leveille}, Michael and {Levenson}, Nancy and {Levine}, Marie and {Levy}, Zena and {Lewis}, Dan and {Lewis}, Hannah and {Libralato}, Mattia and {Lightsey}, Paul and {Link}, Miranda and {Liu}, Lily and {Lo}, Amy and {Lockwood}, Alexandra and {Logue}, Ryan and {Long}, Chris and {Long}, Douglas and {Loomis}, Charles and {Lopez-Caniego}, Marcos and {Alvarez}, Jose Lorenzo and {Love-Pruitt}, Jennifer and {Lucy}, Adrian and {Luetzgendorf}, Nora and {Maghami}, Peiman and {Maiolino}, Roberto and {Major}, Melissa and {Malla}, Sunita and {Malumuth}, Eliot and {Manjavacas}, Elena and {Mannfolk}, Crystal and {Marrione}, Amanda and {Marston}, Anthony and {Martel}, Andr{\'e} and {Maschmann}, Marc and {Masci}, Gregory and {Masciarelli}, Michaela and {Maszkiewicz}, Michael and {Mather}, John and {McKenzie}, Kenny and {McLean}, Brian and {McMaster}, Matthew and {Melbourne}, Katie and {Mel{\'e}ndez}, Marcio and {Menzel}, Michael and {Merz}, Kaiya and {Meyett}, Michele and {Meza}, Luis and {Miskey}, Cherie and {Misselt}, Karl and {Moller}, Christopher and {Morrison}, Jane and {Morse}, Ernie and {Moseley}, Harvey and {Mosier}, Gary and {Mountain}, Matt and {Mueckay}, Julio and {Mueller}, Michael and {Mullally}, Susan and {Murphy}, Jess and {Murray}, Katherine and {Murray}, Claire and {Mustelier}, David and {Muzerolle}, James and {Mycroft}, Matthew and {Myers}, Richard and {Myrick}, Kaila and {Nanavati}, Shashvat and {Nance}, Elizabeth and {Nayak}, Omnarayani and {Naylor}, Bret and {Nelan}, Edmund and {Nickson}, Bryony and {Nielson}, Alethea and {Nieto-Santisteban}, Maria and {Nikolov}, Nikolay and {Noriega-Crespo}, Alberto and {O'Shaughnessy}, Brian and {O'Sullivan}, Brian and {Ochs}, William and {Ogle}, Patrick and {Oleszczuk}, Brenda and {Olmsted}, Joseph and {Osborne}, Shannon and {Ottens}, Richard and {Owens}, Beverly and {Pacifici}, Camilla and {Pagan}, Alyssa and {Page}, James and {Park}, Sang and {Parrish}, Keith and {Patapis}, Polychronis and {Paul}, Lee and {Pauly}, Tyler and {Pavlovsky}, Cheryl and {Pedder}, Andrew and {Peek}, Matthew and {Pena-Guerrero}, Maria and {Pennanen}, Konstantin and {Perez}, Yesenia and {Perna}, Michele and {Perriello}, Beth and {Phillips}, Kevin and {Pietraszkiewicz}, Martin and {Pinaud}, Jean-Paul and {Pirzkal}, Norbert and {Pitman}, Joseph and {Piwowar}, Aidan and {Platais}, Vera and {Player}, Danielle and {Plesha}, Rachel and {Pollizi}, Joe and {Polster}, Ethan and {Pontoppidan}, Klaus and {Porterfield}, Blair and {Proffitt}, Charles and {Pueyo}, Laurent and {Pulliam}, Christine and {Quirt}, Brian and {Quispe Neira}, Irma and {Ramos Alarcon}, Rafael and {Ramsay}, Leah and {Rapp}, Greg and {Rapp}, Robert and {Rauscher}, Bernard and {Ravindranath}, Swara and {Rawle}, Timothy and {Regan}, Michael and {Reichard}, Timothy A. and {Reis}, Carl and {Ressler}, Michael E. and {Rest}, Armin and {Reynolds}, Paul and {Rhue}, Timothy and {Richon}, Karen and {Rickman}, Emily and {Ridgaway}, Michael and {Ritchie}, Christine and {Rix}, Hans-Walter and {Robberto}, Massimo and {Robinson}, Gregory and {Robinson}, Michael and {Robinson}, Orion and {Rock}, Frank and {Rodriguez}, David and {Rodriguez Del Pino}, Bruno and {Roellig}, Thomas and {Rohrbach}, Scott and {Roman}, Anthony and {Romelfanger}, Fred and {Rose}, Perry and {Roteliuk}, Anthony and {Roth}, Marc and {Rothwell}, Braden and {Rowlands}, Neil and {Roy}, Arpita and {Royer}, Pierre and {Royle}, Patricia and {Rui}, Chunlei and {Rumler}, Peter and {Runnels}, Joel and {Russ}, Melissa and {Rustamkulov}, Zafar and {Ryden}, Grant and {Ryer}, Holly and {Sabata}, Modhumita and {Sabatke}, Derek and {Sabbi}, Elena and {Samuelson}, Bridget and {Sapp}, Benjamin and {Sappington}, Bradley and {Sargent}, B. and {Sauer}, Arne and {Scheithauer}, Silvia and {Schlawin}, Everett and {Schlitz}, Joseph and {Schmitz}, Tyler and {Schneider}, Analyn and {Schreiber}, J{\"u}rgen and {Schulze}, Vonessa and {Schwab}, Ryan and {Scott}, John and {Sembach}, Kenneth and {Shanahan}, Clare and {Shaughnessy}, Bryan and {Shaw}, Richard and {Shawger}, Nanci and {Shay}, Christopher and {Sheehan}, Evan and {Shen}, Sharon and {Sherman}, Allan and {Shiao}, Bernard and {Shih}, Hsin-Yi and {Shivaei}, Irene and {Sienkiewicz}, Matthew and {Sing}, David and {Sirianni}, Marco and {Sivaramakrishnan}, Anand and {Skipper}, Joy and {Sloan}, Gregory and {Slocum}, Christine and {Slowinski}, Steven and {Smith}, Erin and {Smith}, Eric and {Smith}, Denise and {Smith}, Corbett and {Snyder}, Gregory and {Soh}, Warren and {Sohn}, Tony and {Soto}, Christian and {Spencer}, Richard and {Stallcup}, Scott and {Stansberry}, John and {Starr}, Carl and {Starr}, Elysia and {Stewart}, Alphonso and {Stiavelli}, Massimo and {Straughn}, Amber and {Strickland}, David and {Stys}, Jeff and {Summers}, Francis and {Sun}, Fengwu and {Sunnquist}, Ben and {Swade}, Daryl and {Swam}, Michael and {Swaters}, Robert and {Swoish}, Robby and {Taylor}, Joanna M. and {Taylor}, Rolanda and {Te Plate}, Maurice and {Tea}, Mason and {Teague}, Kelly and {Telfer}, Randal and {Temim}, Tea and {Thatte}, Deepashri and {Thompson}, Christopher and {Thompson}, Linda and {Thomson}, Shaun and {Tikkanen}, Tuomo and {Tippet}, William and {Todd}, Connor and {Toolan}, Sharon and {Tran}, Hien and {Trejo}, Edwin and {Truong}, Justin and {Tsukamoto}, Chris and {Tustain}, Samuel and {Tyra}, Harrison and {Ubeda}, Leonardo and {Underwood}, Kelli and {Uzzo}, Michael and {Van Campen}, Julie and {Vandal}, Thomas and {Vandenbussche}, Bart and {Vila}, Bego{\~n}a and {Volk}, Kevin and {Wahlgren}, Glenn and {Waldman}, Mark and {Walker}, Chanda and {Wander}, Michel and {Warfield}, Christine and {Warner}, Gerald and {Wasiak}, Matthew and {Watkins}, Mitchell and {Weaver}, Andrew and {Weilert}, Mark and {Weiser}, Nick and {Weiss}, Ben and {Weissman}, Sarah and {Welty}, Alan and {West}, Garrett and {Wheate}, Lauren and {Wheatley}, Elizabeth and {Wheeler}, Thomas and {White}, Rick and {Whiteaker}, Kevin and {Whitehouse}, Paul and {Whiteleather}, Jennifer and {Whitman}, William and {Williams}, Christina and {Willmer}, Christopher and {Willoughby}, Scott and {Wilson}, Andrew and {Wirth}, Gregory and {Wislowski}, Emily and {Wolf}, Erin and {Wolfe}, David and {Wolff}, Schuyler and {Workman}, Bill and {Wright}, Ray and {Wu}, Carl and {Wu}, Rai and {Wymer}, Kristen and {Yates}, Kayla and {Yeager}, Christopher and {Yeates}, Jared and {Yerger}, Ethan and {Yoon}, Jinmi and {Young}, Alice and {Yu}, Susan and {Zak}, Dean and {Zeidler}, Peter and {Zhou}, Julia and {Zielinski}, Thomas and {Zincke}, Cristian and {Zonak}, Stephanie},
        title = "{Characterization of JWST science performance from commissioning}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2022,
        month = jul,
          eid = {arXiv:2207.05632},
        pages = {arXiv:2207.05632},
archivePrefix = {arXiv},
       eprint = {2207.05632},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220705632R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Gobat2012,
       author = {{Gobat}, R. and {Strazzullo}, V. and {Daddi}, E. and {Onodera}, M. and {Renzini}, A. and {B{\'e}thermin}, M. and {Dickinson}, M. and {Carollo}, M. and {Cimatti}, A.},
        title = "{The Early Early Type: Discovery of a Passive Galaxy at z $_{spec}$ \raisebox{-0.5ex}\textasciitilde 3}",
      journal = {\apjl},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2012,
        month = nov,
       volume = {759},
       number = {2},
          eid = {L44},
        pages = {L44},
          doi = {10.1088/2041-8205/759/2/L44},
archivePrefix = {arXiv},
       eprint = {1210.4299},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012ApJ...759L..44G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Kokorev2021,
       author = {{Kokorev}, Vasily I. and {Magdis}, Georgios E. and {Davidzon}, Iary and {Brammer}, Gabriel and {Valentino}, Francesco and {Daddi}, Emanuele and {Ciesla}, Laure and {Liu}, Daizhong and {Jin}, Shuowen and {Cortzen}, Isabella and {Delvecchio}, Ivan and {Gim{\'e}nez-Arteaga}, Clara and {G{\'o}mez-Guijarro}, Carlos and {Sargent}, Mark and {Toft}, Sune and {Weaver}, John R.},
        title = "{The Evolving Interstellar Medium of Star-forming Galaxies, as Traced by Stardust}",
      journal = {\apj},
     keywords = {High-redshift galaxies, Submillimeter astronomy, Infrared astronomy, Astronomy software, Galaxies, Active galaxies, Starburst galaxies, 734, 1647, 786, 1855, 573, 17, 1570, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = nov,
       volume = {921},
       number = {1},
          eid = {40},
        pages = {40},
          doi = {10.3847/1538-4357/ac18ce},
archivePrefix = {arXiv},
       eprint = {2109.06209},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...921...40K},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Liu2019_A3COSMOS,
       author = {{Liu}, Daizhong and {Lang}, P. and {Magnelli}, B. and {Schinnerer}, E. and {Leslie}, S. and {Fudamoto}, Y. and {Bondi}, M. and {Groves}, B. and {Jim{\'e}nez-Andrade}, E. and {Harrington}, K. and {Karim}, A. and {Oesch}, P.~A. and {Sargent}, M. and {Vardoulaki}, E. and {B{\v{a}}descu}, T. and {Moser}, L. and {Bertoldi}, F. and {Battisti}, A. and {da Cunha}, E. and {Zavala}, J. and {Vaccari}, M. and {Davidzon}, I. and {Riechers}, D. and {Aravena}, M.},
        title = "{Automated Mining of the ALMA Archive in the COSMOS Field (A$^{3}$COSMOS). I. Robust ALMA Continuum Photometry Catalogs and Stellar Mass and Star Formation Properties for {\ensuremath{\sim}}700 Galaxies at z = 0.5-6}",
      journal = {\apjs},
     keywords = {galaxies: evolution, galaxies: ISM, galaxies: photometry, galaxies: star formation, submillimeter: galaxies, techniques: photometric, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2019,
        month = oct,
       volume = {244},
       number = {2},
          eid = {40},
        pages = {40},
          doi = {10.3847/1538-4365/ab42da},
archivePrefix = {arXiv},
       eprint = {1910.12872},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJS..244...40L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{Pope2019,
       author = {{Pope}, Alexandra and {Aretxaga}, Itziar and {Hughes}, David and {Wilson}, Grant and {Yun}, Min},
        title = "{TolTEC/LMT Extragalactic Legacy Surveys: Completing our Census of Dust-Obscured Star Formation}",
    booktitle = {American Astronomical Society Meeting Abstracts \#233},
         year = 2019,
       series = {American Astronomical Society Meeting Abstracts},
       volume = {233},
        month = jan,
          eid = {363.20},
        pages = {363.20},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019AAS...23336320P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Wang2019,
       author = {{Wang}, T. and {Schreiber}, C. and {Elbaz}, D. and {Yoshimura}, Y. and {Kohno}, K. and {Shu}, X. and {Yamaguchi}, Y. and {Pannella}, M. and {Franco}, M. and {Huang}, J. and {Lim}, C. -F. and {Wang}, W. -H.},
        title = "{A dominant population of optically invisible massive galaxies in the early Universe}",
      journal = {\nat},
     keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2019,
        month = aug,
       volume = {572},
       number = {7768},
        pages = {211-214},
          doi = {10.1038/s41586-019-1452-4},
archivePrefix = {arXiv},
       eprint = {1908.02372},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019Natur.572..211W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Franco2020,
       author = {{Franco}, M. and {Elbaz}, D. and {Zhou}, L. and {Magnelli}, B. and {Schreiber}, C. and {Ciesla}, L. and {Dickinson}, M. and {Nagar}, N. and {Magdis}, G. and {Alexander}, D.~M. and {B{\'e}thermin}, M. and {Demarco}, R. and {Daddi}, E. and {Wang}, T. and {Mullaney}, J. and {Inami}, H. and {Shu}, X. and {Bournaud}, F. and {Chary}, R. and {Coogan}, R.~T. and {Ferguson}, H. and {Finkelstein}, S.~L. and {Giavalisco}, M. and {G{\'o}mez-Guijarro}, C. and {Iono}, D. and {Juneau}, S. and {Lagache}, G. and {Lin}, L. and {Motohara}, K. and {Okumura}, K. and {Pannella}, M. and {Papovich}, C. and {Pope}, A. and {Rujopakarn}, W. and {Silverman}, J. and {Xiao}, M.},
        title = "{GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies}",
      journal = {\aap},
     keywords = {galaxies: high-redshift, galaxies: evolution, galaxies: star formation, galaxies: photometry, galaxies: fundamental parameters, submillimeter: galaxies, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = nov,
       volume = {643},
          eid = {A53},
        pages = {A53},
          doi = {10.1051/0004-6361/202038310},
archivePrefix = {arXiv},
       eprint = {2005.03040},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...643A..53F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Shu2022,
       author = {{Shu}, Xinwen and {Yang}, Lei and {Liu}, Daizhong and {Wang}, Wei-Hao and {Wang}, Tao and {Han}, Yunkun and {Huang}, Xingxing and {Lim}, Chen-Fatt and {Chang}, Yu-Yen and {Zheng}, Wei and {Zheng}, XianZhong and {Wang}, Junxian and {Kong}, Xu},
        title = "{A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters}",
      journal = {\apj},
     keywords = {412, 734, Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = feb,
       volume = {926},
       number = {2},
          eid = {155},
        pages = {155},
          doi = {10.3847/1538-4357/ac3de5},
archivePrefix = {arXiv},
       eprint = {2112.03709},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...926..155S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Zhou2020,
       author = {{Zhou}, L. and {Elbaz}, D. and {Franco}, M. and {Magnelli}, B. and {Schreiber}, C. and {Wang}, T. and {Ciesla}, L. and {Daddi}, E. and {Dickinson}, M. and {Nagar}, N. and {Magdis}, G. and {Alexander}, D.~M. and {B{\'e}thermin}, M. and {Demarco}, R. and {Mullaney}, J. and {Bournaud}, F. and {Ferguson}, H. and {Finkelstein}, S.~L. and {Giavalisco}, M. and {Inami}, H. and {Iono}, D. and {Juneau}, S. and {Lagache}, G. and {Messias}, H. and {Motohara}, K. and {Okumura}, K. and {Pannella}, M. and {Papovich}, C. and {Pope}, A. and {Rujopakarn}, W. and {Shi}, Y. and {Shu}, X. and {Silverman}, J.},
        title = "{GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5}",
      journal = {\aap},
     keywords = {galaxies: high-redshift, galaxies: evolution, galaxies: star formation, galaxies: photometry, galaxies: structure, submillimeter: galaxies, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = oct,
       volume = {642},
          eid = {A155},
        pages = {A155},
          doi = {10.1051/0004-6361/202038059},
archivePrefix = {arXiv},
       eprint = {2008.08518},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...642A.155Z},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021Natur.597..489F,
       author = {{Fudamoto}, Y. and {Oesch}, P.~A. and {Schouws}, S. and {Stefanon}, M. and {Smit}, R. and {Bouwens}, R.~J. and {Bowler}, R.~A.~A. and {Endsley}, R. and {Gonzalez}, V. and {Inami}, H. and {Labbe}, I. and {Stark}, D. and {Aravena}, M. and {Barrufet}, L. and {da Cunha}, E. and {Dayal}, P. and {Ferrara}, A. and {Graziani}, L. and {Hodge}, J. and {Hutter}, A. and {Li}, Y. and {De Looze}, I. and {Nanayakkara}, T. and {Pallottini}, A. and {Riechers}, D. and {Schneider}, R. and {Ucci}, G. and {van der Werf}, P. and {White}, C.},
        title = "{Normal, dust-obscured galaxies in the epoch of reionization}",
      journal = {\nat},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = sep,
       volume = {597},
       number = {7877},
        pages = {489-492},
          doi = {10.1038/s41586-021-03846-z},
archivePrefix = {arXiv},
       eprint = {2109.10378},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021Natur.597..489F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Fudamoto2021,
       author = {{Fudamoto}, Y. and {Oesch}, P.~A. and {Schouws}, S. and {Stefanon}, M. and {Smit}, R. and {Bouwens}, R.~J. and {Bowler}, R.~A.~A. and {Endsley}, R. and {Gonzalez}, V. and {Inami}, H. and {Labbe}, I. and {Stark}, D. and {Aravena}, M. and {Barrufet}, L. and {da Cunha}, E. and {Dayal}, P. and {Ferrara}, A. and {Graziani}, L. and {Hodge}, J. and {Hutter}, A. and {Li}, Y. and {De Looze}, I. and {Nanayakkara}, T. and {Pallottini}, A. and {Riechers}, D. and {Schneider}, R. and {Ucci}, G. and {van der Werf}, P. and {White}, C.},
        title = "{Normal, dust-obscured galaxies in the epoch of reionization}",
      journal = {\nat},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = sep,
       volume = {597},
       number = {7877},
        pages = {489-492},
          doi = {10.1038/s41586-021-03846-z},
archivePrefix = {arXiv},
       eprint = {2109.10378},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021Natur.597..489F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Sun2021,
       author = {{Sun}, Fengwu and {Egami}, Eiichi and {P{\'e}rez-Gonz{\'a}lez}, Pablo G. and {Smail}, Ian and {Caputi}, Karina I. and {Bauer}, Franz E. and {Rawle}, Timothy D. and {Fujimoto}, Seiji and {Kohno}, Kotaro and {Dudzevi{\v{c}}i{\={u}}t{\.{e}}}, Ugn{\.{e}} and {Atek}, Hakim and {Bianconi}, Matteo and {Chapman}, Scott C. and {Combes}, Francoise and {Jauzac}, Mathilde and {Jolly}, Jean-Baptiste and {Koekemoer}, Anton M. and {Magdis}, Georgios E. and {Rodighiero}, Giulia and {Rujopakarn}, Wiphu and {Schaerer}, Daniel and {Steinhardt}, Charles L. and {Van der Werf}, Paul and {Walth}, Gregory L. and {Weaver}, John R.},
        title = "{Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters}",
      journal = {\apj},
     keywords = {594, 790, 734, 1570, 670, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = dec,
       volume = {922},
       number = {2},
          eid = {114},
        pages = {114},
          doi = {10.3847/1538-4357/ac2578},
archivePrefix = {arXiv},
       eprint = {2109.01751},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...922..114S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Marsan2022,
       author = {{Marsan}, Z. Cemile and {Muzzin}, Adam and {Marchesini}, Danilo and {Stefanon}, Mauro and {Martis}, Nicholas and {Annunziatella}, Marianna and {Chan}, Jeffrey C.~C. and {Cooper}, Michael C. and {Forrest}, Ben and {Gomez}, Percy and {McConachie}, Ian and {Wilson}, Gillian},
        title = "{The Number Densities and Stellar Populations of Massive Galaxies at 3 < z < 6: A Diverse, Rapidly Forming Population in the Early Universe}",
      journal = {\apj},
     keywords = {594},
         year = 2022,
        month = jan,
       volume = {924},
       number = {1},
          eid = {25},
        pages = {25},
          doi = {10.3847/1538-4357/ac312a},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...924...25M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Schreiber2018,
       author = {{Schreiber}, C. and {Labb{\'e}}, I. and {Glazebrook}, K. and {Bekiaris}, G. and {Papovich}, C. and {Costa}, T. and {Elbaz}, D. and {Kacprzak}, G.~G. and {Nanayakkara}, T. and {Oesch}, P. and {Pannella}, M. and {Spitler}, L. and {Straatman}, C. and {Tran}, K. -V. and {Wang}, T.},
        title = "{Jekyll \& Hyde: quiescence and extreme obscuration in a pair of massive galaxies 1.5 Gyr after the Big Bang}",
      journal = {\aap},
     keywords = {galaxies: evolution, galaxies: high-redshift, galaxies: kinematics and dynamics, galaxies: star formation, galaxies: stellar content, sub-millimeter: galaxies, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = mar,
       volume = {611},
          eid = {A22},
        pages = {A22},
          doi = {10.1051/0004-6361/201731917},
archivePrefix = {arXiv},
       eprint = {1709.03505},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018A&A...611A..22S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Casey2014,
       author = {{Casey}, Caitlin M. and {Narayanan}, Desika and {Cooray}, Asantha},
        title = "{Dusty star-forming galaxies at high redshift}",
      journal = {\physrep},
     keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2014,
        month = aug,
       volume = {541},
       number = {2},
        pages = {45-161},
          doi = {10.1016/j.physrep.2014.02.009},
archivePrefix = {arXiv},
       eprint = {1402.1456},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014PhR...541...45C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Zavala2021,
       author = {{Zavala}, J.~A. and {Casey}, C.~M. and {Manning}, S.~M. and {Aravena}, M. and {Bethermin}, M. and {Caputi}, K.~I. and {Clements}, D.~L. and {Cunha}, E. da and {Drew}, P. and {Finkelstein}, S.~L. and {Fujimoto}, S. and {Hayward}, C. and {Hodge}, J. and {Kartaltepe}, J.~S. and {Knudsen}, K. and {Koekemoer}, A.~M. and {Long}, A.~S. and {Magdis}, G.~E. and {Man}, A.~W.~S. and {Popping}, G. and {Sanders}, D. and {Scoville}, N. and {Sheth}, K. and {Staguhn}, J. and {Toft}, S. and {Treister}, E. and {Vieira}, J.~D. and {Yun}, M.~S.},
        title = "{The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years}",
      journal = {\apj},
     keywords = {Galaxy evolution, Galaxies, Dust continuum emission, Millimeter astronomy, Submillimeter astronomy, Star formation, High-redshift galaxies, Surveys, Galaxy counts, Luminosity function, 594, 573, 412, 1061, 1647, 1569, 734, 1671, 588, 942, Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = mar,
       volume = {909},
       number = {2},
          eid = {165},
        pages = {165},
          doi = {10.3847/1538-4357/abdb27},
archivePrefix = {arXiv},
       eprint = {2101.04734},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...909..165Z},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Manning2022,
       author = {{Manning}, Sinclaire M. and {Casey}, Caitlin M. and {Zavala}, Jorge A. and {Magdis}, Georgios E. and {Drew}, Patrick M. and {Champagne}, Jaclyn B. and {Aravena}, Manuel and {B{\'e}thermin}, Matthieu and {Clements}, David L. and {Finkelstein}, Steven L. and {Fujimoto}, Seiji and {Hayward}, Christopher C. and {Hodge}, Jacqueline A. and {Ilbert}, Olivier and {Kartaltepe}, Jeyhan S. and {Knudsen}, Kirsten K. and {Koekemoer}, Anton M. and {Man}, Allison W.~S. and {Sanders}, David B. and {Sheth}, Kartik and {Spilker}, Justin S. and {Staguhn}, Johannes and {Talia}, Margherita and {Treister}, Ezequiel and {Yun}, Min S.},
        title = "{Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies}",
      journal = {\apj},
     keywords = {1570, 734, 412, Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = jan,
       volume = {925},
       number = {1},
          eid = {23},
        pages = {23},
          doi = {10.3847/1538-4357/ac366a},
archivePrefix = {arXiv},
       eprint = {2111.02428},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...925...23M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Glazebrook2017,
       author = {{Glazebrook}, Karl and {Schreiber}, Corentin and {Labb{\'e}}, Ivo and {Nanayakkara}, Themiya and {Kacprzak}, Glenn G. and {Oesch}, Pascal A. and {Papovich}, Casey and {Spitler}, Lee R. and {Straatman}, Caroline M.~S. and {Tran}, Kim-Vy H. and {Yuan}, Tiantian},
        title = "{A massive, quiescent galaxy at a redshift of 3.717}",
      journal = {\nat},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = apr,
       volume = {544},
       number = {7648},
        pages = {71-74},
          doi = {10.1038/nature21680},
archivePrefix = {arXiv},
       eprint = {1702.01751},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017Natur.544...71G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Fontanot2009,
       author = {{Fontanot}, Fabio and {De Lucia}, Gabriella and {Monaco}, Pierluigi and {Somerville}, Rachel S. and {Santini}, Paola},
        title = "{The many manifestations of downsizing: hierarchical galaxy formation models confront observations}",
      journal = {\mnras},
     keywords = {galaxies: evolution, galaxies: formation, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2009,
        month = aug,
       volume = {397},
       number = {4},
        pages = {1776-1790},
          doi = {10.1111/j.1365-2966.2009.15058.x},
archivePrefix = {arXiv},
       eprint = {0901.1130},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2009MNRAS.397.1776F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Toft2017,
       author = {{Toft}, Sune and {Zabl}, Johannes and {Richard}, Johan and {Gallazzi}, Anna and {Zibetti}, Stefano and {Prescott}, Moire and {Grillo}, Claudio and {Man}, Allison W.~S. and {Lee}, Nicholas Y. and {G{\'o}mez-Guijarro}, Carlos and {Stockmann}, Mikkel and {Magdis}, Georgios and {Steinhardt}, Charles L.},
        title = "{A massive, dead disk galaxy in the early Universe}",
      journal = {\nat},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = jun,
       volume = {546},
       number = {7659},
        pages = {510-513},
          doi = {10.1038/nature22388},
archivePrefix = {arXiv},
       eprint = {1706.07030},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017Natur.546..510T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Akhshik2022,
       author = {{Akhshik}, Mohammad and {Whitaker}, Katherine E. and {Leja}, Joel and {Richard}, Johan and {Spilker}, Justin S. and {Song}, Mimi and {Brammer}, Gabriel and {Bezanson}, Rachel and {Ebeling}, Harald and {Gallazzi}, Anna R. and {Mahler}, Guillaume and {Mowla}, Lamiya A. and {Nelson}, Erica J. and {Pacifici}, Camilla and {Sharon}, Keren and {Toft}, Sune and {Williams}, Christina C. and {Wright}, Lillian and {Zabl}, Johannes},
        title = "{REQUIEM-2D: A diversity of formation pathways in a sample of spatially-resolved massive quiescent galaxies at z\raisebox{-0.5ex}\textasciitilde2}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = mar,
          eid = {arXiv:2203.04979},
        pages = {arXiv:2203.04979},
archivePrefix = {arXiv},
       eprint = {2203.04979},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220304979A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Whitaker2021,
       author = {{Whitaker}, Katherine E. and {Williams}, Christina C. and {Mowla}, Lamiya and {Spilker}, Justin S. and {Toft}, Sune and {Narayanan}, Desika and {Pope}, Alexandra and {Magdis}, Georgios E. and {van Dokkum}, Pieter G. and {Akhshik}, Mohammad and {Bezanson}, Rachel and {Brammer}, Gabriel B. and {Leja}, Joel and {Man}, Allison and {Nelson}, Erica J. and {Richard}, Johan and {Pacifici}, Camilla and {Sharon}, Keren and {Valentino}, Francesco},
        title = "{Quenching of star formation from a lack of inflowing gas to galaxies}",
      journal = {\nat},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2021,
        month = sep,
       volume = {597},
       number = {7877},
        pages = {485-488},
          doi = {10.1038/s41586-021-03806-7},
archivePrefix = {arXiv},
       eprint = {2109.10384},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021Natur.597..485W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Tanaka2019,
       author = {{Tanaka}, Masayuki and {Valentino}, Francesco and {Toft}, Sune and {Onodera}, Masato and {Shimakawa}, Rhythm and {Ceverino}, Daniel and {Faisst}, Andreas L. and {Gallazzi}, Anna and {G{\'o}mez-Guijarro}, Carlos and {Kubo}, Mariko and {Magdis}, Georgios E. and {Steinhardt}, Charles L. and {Stockmann}, Mikkel and {Yabe}, Kiyoto and {Zabl}, Johannes},
        title = "{Stellar Velocity Dispersion of a Massive Quenching Galaxy at z = 4.01}",
      journal = {\apjl},
     keywords = {Galaxy formation, Galaxy evolution, Elliptical galaxies, Galaxy dynamics, High-redshift galaxies, 595, 594, 456, 591, 734, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = nov,
       volume = {885},
       number = {2},
          eid = {L34},
        pages = {L34},
          doi = {10.3847/2041-8213/ab4ff3},
archivePrefix = {arXiv},
       eprint = {1909.10721},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...885L..34T},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Hill2017,
       author = {{Hill}, Allison R. and {Muzzin}, Adam and {Franx}, Marijn and {Clauwens}, Bart and {Schreiber}, Corentin and {Marchesini}, Danilo and {Stefanon}, Mauro and {Labbe}, Ivo and {Brammer}, Gabriel and {Caputi}, Karina and {Fynbo}, Johan and {Milvang-Jensen}, Bo and {Skelton}, Rosalind E. and {van Dokkum}, Pieter and {Whitaker}, Katherine E.},
        title = "{The Mass, Color, and Structural Evolution of Today{\textquoteright}s Massive Galaxies Since z {\ensuremath{\sim}} 5}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: structure, Astrophysics - Astrophysics of Galaxies},
         year = 2017,
        month = mar,
       volume = {837},
       number = {2},
          eid = {147},
        pages = {147},
          doi = {10.3847/1538-4357/aa61fe},
archivePrefix = {arXiv},
       eprint = {1702.06126},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017ApJ...837..147H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Caputi2011,
       author = {{Caputi}, K.~I. and {Cirasuolo}, M. and {Dunlop}, J.~S. and {McLure}, R.~J. and {Farrah}, D. and {Almaini}, O.},
        title = "{The stellar mass function of the most-massive galaxies at 3 {\ensuremath{\leq}}z < 5 in the UKIDSS Ultra Deep Survey}",
      journal = {\mnras},
     keywords = {galaxies: luminosity function, mass function, galaxies: statistics, infrared: galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2011,
        month = may,
       volume = {413},
       number = {1},
        pages = {162-176},
          doi = {10.1111/j.1365-2966.2010.18118.x},
archivePrefix = {arXiv},
       eprint = {1008.5244},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2011MNRAS.413..162C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Carnall2018,
       author = {{Carnall}, A.~C. and {McLure}, R.~J. and {Dunlop}, J.~S. and {Dav{\'e}}, R.},
        title = "{Inferring the star formation histories of massive quiescent galaxies with BAGPIPES: evidence for multiple quenching mechanisms}",
      journal = {\mnras},
     keywords = {methods: statistical, galaxies: evolution, galaxies: star formation, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2018,
        month = nov,
       volume = {480},
       number = {4},
        pages = {4379-4401},
          doi = {10.1093/mnras/sty2169},
archivePrefix = {arXiv},
       eprint = {1712.04452},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.4379C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Retzlaff2010,
       author = {{Retzlaff}, J. and {Rosati}, P. and {Dickinson}, M. and {Vandame}, B. and {Rit{\'e}}, C. and {Nonino}, M. and {Cesarsky}, C. and {GOODS Team}},
        title = "{The Great Observatories Origins Deep Survey. VLT/ISAAC near-infrared imaging of the GOODS-South field}",
      journal = {\aap},
     keywords = {cosmology: observations, large-scale structure of the Universe, galaxies: evolution, infrared: galaxies, surveys, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2010,
        month = feb,
       volume = {511},
          eid = {A50},
        pages = {A50},
          doi = {10.1051/0004-6361/200912940},
archivePrefix = {arXiv},
       eprint = {0912.1306},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010A&A...511A..50R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Fontana2014,
       author = {{Fontana}, A. and {Dunlop}, J.~S. and {Paris}, D. and {Targett}, T.~A. and {Boutsia}, K. and {Castellano}, M. and {Galametz}, A. and {Grazian}, A. and {McLure}, R. and {Merlin}, E. and {Pentericci}, L. and {Wuyts}, S. and {Almaini}, O. and {Caputi}, K. and {Chary}, R. -R. and {Cirasuolo}, M. and {Conselice}, C.~J. and {Cooray}, A. and {Daddi}, E. and {Dickinson}, M. and {Faber}, S.~M. and {Fazio}, G. and {Ferguson}, H.~C. and {Giallongo}, E. and {Giavalisco}, M. and {Grogin}, N.~A. and {Hathi}, N. and {Koekemoer}, A.~M. and {Koo}, D.~C. and {Lucas}, R.~A. and {Nonino}, M. and {Rix}, H.~W. and {Renzini}, A. and {Rosario}, D. and {Santini}, P. and {Scarlata}, C. and {Sommariva}, V. and {Stark}, D.~P. and {van der Wel}, A. and {Vanzella}, E. and {Wild}, V. and {Yan}, H. and {Zibetti}, S.},
        title = "{The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts}",
      journal = {\aap},
     keywords = {surveys, galaxies: evolution, Astrophysics - Astrophysics of Galaxies},
         year = 2014,
        month = oct,
       volume = {570},
          eid = {A11},
        pages = {A11},
          doi = {10.1051/0004-6361/201423543},
archivePrefix = {arXiv},
       eprint = {1409.7082},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014A&A...570A..11F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Ito2022,
       author = {{Ito}, Kei and {Tanaka}, Masayuki and {Miyaji}, Takamitsu and {Ilbert}, Olivier and {Kauffmann}, Olivier B. and {Koekemoer}, Anton M. and {Marchesi}, Stefano and {Shuntov}, Marko and {Toft}, Sune and {Valentino}, Francesco and {Weaver}, John R.},
        title = "{COSMOS2020: Ubiquitous AGN Activity of Massive Quiescent Galaxies at $0<z<5$ Revealed by X-ray and Radio Stacking}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = mar,
          eid = {arXiv:2203.04322},
        pages = {arXiv:2203.04322},
archivePrefix = {arXiv},
       eprint = {2203.04322},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220304322I},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Lower2020,
       author = {{Lower}, Sidney and {Narayanan}, Desika and {Leja}, Joel and {Johnson}, Benjamin D. and {Conroy}, Charlie and {Dav{\'e}}, Romeel},
        title = "{How Well Can We Measure the Stellar Mass of a Galaxy: The Impact of the Assumed Star Formation History Model in SED Fitting}",
      journal = {\apj},
     keywords = {Astronomy data modeling, Hydrodynamical simulations, Stellar masses, Galaxy properties, Spectral energy distribution, Radiative transfer simulations, 1859, 767, 1614, 615, 2129, 1967, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = nov,
       volume = {904},
       number = {1},
          eid = {33},
        pages = {33},
          doi = {10.3847/1538-4357/abbfa7},
archivePrefix = {arXiv},
       eprint = {2006.03599},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...904...33L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Marrone2018,
       author = {{Marrone}, D.~P. and {Spilker}, J.~S. and {Hayward}, C.~C. and {Vieira}, J.~D. and {Aravena}, M. and {Ashby}, M.~L.~N. and {Bayliss}, M.~B. and {B{\'e}thermin}, M. and {Brodwin}, M. and {Bothwell}, M.~S. and {Carlstrom}, J.~E. and {Chapman}, S.~C. and {Chen}, Chian-Chou and {Crawford}, T.~M. and {Cunningham}, D.~J.~M. and {De Breuck}, C. and {Fassnacht}, C.~D. and {Gonzalez}, A.~H. and {Greve}, T.~R. and {Hezaveh}, Y.~D. and {Lacaille}, K. and {Litke}, K.~C. and {Lower}, S. and {Ma}, J. and {Malkan}, M. and {Miller}, T.~B. and {Morningstar}, W.~R. and {Murphy}, E.~J. and {Narayanan}, D. and {Phadke}, K.~A. and {Rotermund}, K.~M. and {Sreevani}, J. and {Stalder}, B. and {Stark}, A.~A. and {Strandet}, M.~L. and {Tang}, M. and {Wei{\ss}}, A.},
        title = "{Galaxy growth in a massive halo in the first billion years of cosmic history}",
      journal = {\nat},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = jan,
       volume = {553},
       number = {7686},
        pages = {51-54},
          doi = {10.1038/nature24629},
archivePrefix = {arXiv},
       eprint = {1712.03020},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018Natur.553...51M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{2021jwst.prop.2285C,
       author = {{Carnall}, Adam and {Begley}, Ryan Anthony and {Cimatti}, Andrea and {Cullen}, Fergus and {Dunlop}, James S. and {Hamadouche}, Massissilia Louisa and {McLeod}, Derek and {McLure}, Ross and {Walker}, Sam and {Wild}, Vivienne},
        title = "{A massive quiescent galaxy at redshift 4.657}",
 howpublished = {JWST Proposal. Cycle 1},
         year = 2021,
        month = mar,
        pages = {2285},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021jwst.prop.2285C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{2021jwst.prop.2565G,
       author = {{Glazebrook}, Karl and {Nanayakkara}, Themiya and {Esdaile}, James and {Espejo}, Juan Manuel and {Jacobs}, Colin and {Kacprzak}, Glenn G. and {Labbe}, Ivo and {Marchesini}, Danilo and {Marsan}, Cemile and {Oesch}, Pascal and {Papovich}, Casey and {Remus}, Rhea-Silvia and {Schreiber}, Corentin and {Straatman}, Caroline and {Tran}, Kim-Vy and {Urbina}, Claudia Lagos},
        title = "{How Many Quiescent Galaxies are There at 3}",
 howpublished = {JWST Proposal. Cycle 1},
         year = 2021,
        month = mar,
        pages = {2565},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021jwst.prop.2565G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{2021jwst.prop.2198B,
       author = {{Barrufet}, Laia and {Oesch}, Pascal and {Fudamoto}, Yoshinobu and {Illingworth}, Garth D. and {Labbe}, Ivo and {Magee}, Daniel K. and {Stefanon}, Mauro and {van Dokkum}, Pieter},
        title = "{Quiescent or dusty? Unveiling the nature of extremely red galaxies at z>3}",
 howpublished = {JWST Proposal. Cycle 1},
         year = 2021,
        month = mar,
        pages = {2198},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021jwst.prop.2198B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Fudamoto2020,
       author = {{Fudamoto}, Y. and {Oesch}, P.~A. and {Faisst}, A. and {B{\'e}thermin}, M. and {Ginolfi}, M. and {Khusanova}, Y. and {Loiacono}, F. and {Le F{\`e}vre}, O. and {Capak}, P. and {Schaerer}, D. and {Silverman}, J.~D. and {Cassata}, P. and {Yan}, L. and {Amorin}, R. and {Bardelli}, S. and {Boquien}, M. and {Cimatti}, A. and {Dessauges-Zavadsky}, M. and {Fujimoto}, S. and {Gruppioni}, C. and {Hathi}, N.~P. and {Ibar}, E. and {Jones}, G.~C. and {Koekemoer}, A.~M. and {Lagache}, G. and {Lemaux}, B.~C. and {Maiolino}, R. and {Narayanan}, D. and {Pozzi}, F. and {Riechers}, D.~A. and {Rodighiero}, G. and {Talia}, M. and {Toft}, S. and {Vallini}, L. and {Vergani}, D. and {Zamorani}, G. and {Zucca}, E.},
        title = "{The ALPINE-ALMA [CII] survey. Dust attenuation properties and obscured star formation at z {\ensuremath{\sim}} 4.4-5.8}",
      journal = {\aap},
     keywords = {galaxies: high-redshift, galaxies: ISM, dust, extinction, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = nov,
       volume = {643},
          eid = {A4},
        pages = {A4},
          doi = {10.1051/0004-6361/202038163},
archivePrefix = {arXiv},
       eprint = {2004.10760},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...643A...4F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Cowley2019,
       author = {{Cowley}, William I. and {Caputi}, Karina I. and {Deshmukh}, Smaran and {Ashby}, Matthew L.~N. and {Fazio}, Giovanni G. and {Le F{\`e}vre}, Olivier and {Fynbo}, Johan P.~U. and {Ilbert}, Oliver and {Milvang-Jensen}, Bo},
        title = "{The Stellar-to-halo Mass Ratios of Passive and Star-forming Galaxies at z {\ensuremath{\sim}} 2-3 from the SMUVS Survey}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, large-scale structure of universe, methods: statistical, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = apr,
       volume = {874},
       number = {2},
          eid = {114},
        pages = {114},
          doi = {10.3847/1538-4357/ab089b},
archivePrefix = {arXiv},
       eprint = {1901.10455},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...874..114C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Schreiber2020_ARAA,
       author = {{F{\"o}rster Schreiber}, Natascha M. and {Wuyts}, Stijn},
        title = "{Star-Forming Galaxies at Cosmic Noon}",
      journal = {\araa},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = aug,
       volume = {58},
        pages = {661-725},
          doi = {10.1146/annurev-astro-032620-021910},
archivePrefix = {arXiv},
       eprint = {2010.10171},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ARA&A..58..661F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Peng2012,
       author = {{Peng}, Ying-jie and {Lilly}, Simon J. and {Renzini}, Alvio and {Carollo}, Marcella},
        title = "{Mass and Environment as Drivers of Galaxy Evolution. II. The Quenching of Satellite Galaxies as the Origin of Environmental Effects}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: groups: general, galaxies: luminosity function, mass function, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2012,
        month = sep,
       volume = {757},
       number = {1},
          eid = {4},
        pages = {4},
          doi = {10.1088/0004-637X/757/1/4},
archivePrefix = {arXiv},
       eprint = {1106.2546},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2012ApJ...757....4P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Donnari2021a,
       author = {{Donnari}, Martina and {Pillepich}, Annalisa and {Joshi}, Gandhali D. and {Nelson}, Dylan and {Genel}, Shy and {Marinacci}, Federico and {Rodriguez-Gomez}, Vicente and {Pakmor}, R{\"u}diger and {Torrey}, Paul and {Vogelsberger}, Mark and {Hernquist}, Lars},
        title = "{Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing}",
      journal = {\mnras},
     keywords = {methods: numerical, galaxies: evolution, galaxies: formation, galaxies: haloes, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2021,
        month = jan,
       volume = {500},
       number = {3},
        pages = {4004-4024},
          doi = {10.1093/mnras/staa3006},
archivePrefix = {arXiv},
       eprint = {2008.00005},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.500.4004D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{Donnari2021b,
       author = {{Donnari}, Martina and {Pillepich}, Annalisa and {Nelson}, Dylan and {Marinacci}, Federico and {Vogelsberger}, Mark and {Hernquist}, Lars},
        title = "{Quenched fractions in the IllustrisTNG simulations: comparison with observations and other theoretical models}",
      journal = {\mnras},
     keywords = {galaxies: clusters: general, galaxies: evolution, galaxies: formation, galaxies: groups: general, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
         year = 2021,
        month = oct,
       volume = {506},
       number = {4},
        pages = {4760-4780},
          doi = {10.1093/mnras/stab1950},
archivePrefix = {arXiv},
       eprint = {2008.00004},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.506.4760D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Hviding2022,
       author = {{Hviding}, Raphael E. and {Hainline}, Kevin N. and {Rieke}, Marcia and {Juneau}, St{\'e}phanie and {Lyu}, Jianwei and {Pucha}, Ragadeepika},
        title = "{A New Infrared Criterion for Selecting Active Galactic Nuclei to Lower Luminosities}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = mar,
          eid = {arXiv:2203.11217},
        pages = {arXiv:2203.11217},
archivePrefix = {arXiv},
       eprint = {2203.11217},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220311217H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Viero2022,
       author = {{Viero}, Marco P. and {Sun}, Guochao and {Chung}, Dongwoo T. and {Moncelsi}, Lorenzo and {Condon}, Sam S.},
        title = "{The Early Universe was Dust-Rich and Extremely Hot}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = mar,
          eid = {arXiv:2203.14312},
        pages = {arXiv:2203.14312},
archivePrefix = {arXiv},
       eprint = {2203.14312},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220314312V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Shuntov2022,
       author = {{Shuntov}, M. and {McCracken}, H.~J. and {Gavazzi}, R. and {Laigle}, C. and {Weaver}, J.~R. and {Davidzon}, I. and {Ilbert}, O. and {Kauffmann}, O.~B. and {Faisst}, A. and {Dubois}, Y. and {Koekemoer}, A.~M. and {Moneti}, A. and {Milvang-Jensen}, B. and {Mobasher}, B. and {Sanders}, D.~B. and {Toft}, S.},
        title = "{COSMOS2020: Cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z {\ensuremath{\sim}} 5}",
      journal = {\aap},
     keywords = {galaxies: halos, galaxies: evolution, large-scale structure of Universe, Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = aug,
       volume = {664},
          eid = {A61},
        pages = {A61},
          doi = {10.1051/0004-6361/202243136},
archivePrefix = {arXiv},
       eprint = {2203.10895},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022A&A...664A..61S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}



@ARTICLE{Cooper2022,
       author = {{Cooper}, Olivia R. and {Casey}, Caitlin M. and {Zavala}, Jorge A. and {Champagne}, Jaclyn B. and {da Cunha}, Elisabete and {Long}, Arianna S. and {Spilker}, Justin S. and {Staguhn}, Johannes},
        title = "{Searching Far and Long I: Pilot ALMA 2mm Follow-up of Bright Dusty Galaxies as a Redshift Filter}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = mar,
          eid = {arXiv:2203.14973},
        pages = {arXiv:2203.14973},
archivePrefix = {arXiv},
       eprint = {2203.14973},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220314973C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

 @article{Songaila_1994, title={The Hawaii K-Band Galaxy Survey. III. Spectroscopy of K < 20 Galaxies}, volume={94}, ISSN={0067-0049}, DOI={10.1086/192080}, abstractNote={We present spectra and multicolor (B, I, K) data for near-infrared (K) selected spatially complete magnitude limited (K < 20) galaxy samples from the Hawaii Survey. The redshift identification of the sample of 298 galaxies is substantially complete to a B magnitude of 26 and an I magnitude of 22.5, and identification of observed galaxies ranges from nearly 100\% completeness at K < 18 to ~70\% completeness at K = 19-20. We note that many of the unidentified objects appear to be red (I - K) objects which are flat in the optical and spectroscopically featureless. Strengths of spectral-line features and breaks are tabulated for the 262 galaxies with reasonably secure redshifts. The measured redshift is nearly all fall at z <~ 1, with the exception of a compact absorption- line object at z = 2.35. At K <= 18, the redshift distribution is well fitted by a model with no luminosity evolution, implying that from the K- band Hubble diagram, the Hubble constant can vary at most by 10\% over the redshift range from z ~0.025 to 0.25, and that positive luminosity evolution at any significant level between z = 0 and z = 1 is ruled out. However, the evolution of both the emission-line strengths and the 4000 A break indicates that galaxies were undergoing significantly more star formation at z = 1 than at the present time.}, note={ADS Bibcode: 1994ApJS...94..461S}, journal={The Astrophysical Journal Supplement Series}, author={Songaila, A. and Cowie, L. L. and Hu, E. M. and Gardner, J. P.}, year={1994}, month={Oct}, pages={461} }
 
  @article{Glazebrook_1995, title={An imaging K-band survey - II. The redshift survey and galaxy evolution in the infrared}, volume={275}, ISSN={0035-8711}, DOI={10.1093/mnras/275.1.169}, abstractNote={We present further results from an imaging K-band survey of 552 arcmin^2, complete to a 5sigma limit of K~=17.3. This paper describes a redshift survey of 124 galaxies, and addresses the colours of faint galaxies and the evolution of the K-band luminosity function. The optical-to-infrared colours are consistent with the range expected from synthetic galaxy spectra, although there are some cases of very red nuclei. These may possibly be attributed to either extinction or metallicity gradients. Our data show no evidence for evolution of the K-band luminosity function at z<0.5, and the results are well described by a Schechter function with M^*_K=-22.75+/-0.13+5 log_10h and phi*=0.026+/-0.003h^3 Mpc^-3. This is a somewhat higher normalization than has been found by previous workers, and it removes much of the excess in faint K and b_J counts with respect to a no-evolution model. However, we do find evidence for evolution at z>0.5: M^*K is approximately 0.75 mag brighter at z=1. This luminosity evolution is balanced by a reduced normalization at high redshift: the total luminosity density is required to be approximately constant in order not to exceed the faint counts. The overall evolution is thus opposite to that expected in simple merger-dominated models; we briefly consider possible interpretations of this result.}, note={ADS Bibcode: 1995MNRAS.275..169G}, journal={Monthly Notices of the Royal Astronomical Society}, author={Glazebrook, Karl and Peacock, J. A. and Miller, L. and Collins, C. A.}, year={1995}, month={Jul}, pages={169–184} }

@ARTICLE{Ilbert_2010,
       author = {{Ilbert}, O. and {Salvato}, M. and {Le Floc'h}, E. and {Aussel}, H. and {Capak}, P. and {McCracken}, H.~J. and {Mobasher}, B. and {Kartaltepe}, J. and {Scoville}, N. and {Sanders}, D.~B. and {Arnouts}, S. and {Bundy}, K. and {Cassata}, P. and {Kneib}, J. -P. and {Koekemoer}, A. and {Le F{\`e}vre}, O. and {Lilly}, S. and {Surace}, J. and {Taniguchi}, Y. and {Tasca}, L. and {Thompson}, D. and {Tresse}, L. and {Zamojski}, M. and {Zamorani}, G. and {Zucca}, E.},
        title = "{Galaxy Stellar Mass Assembly Between 0.2 < z < 2 from the S-COSMOS Survey}",
      journal = {\apj},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: luminosity function, mass function, Astrophysics - Cosmology and Extragalactic Astrophysics},
         year = 2010,
        month = feb,
       volume = {709},
       number = {2},
        pages = {644-663},
          doi = {10.1088/0004-637X/709/2/644},
archivePrefix = {arXiv},
       eprint = {0903.0102},
 primaryClass = {astro-ph.CO},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010ApJ...709..644I},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Cecchi2019,
       author = {{Cecchi}, Rachele and {Bolzonella}, Micol and {Cimatti}, Andrea and {Girelli}, Giacomo},
        title = "{Quiescent Galaxies at z {\ensuremath{\gtrsim}} 2.5: Observations versus Models}",
      journal = {\apjl},
     keywords = {galaxies: evolution, galaxies: formation, galaxies: high-redshift, galaxies: star formation, galaxies: photometry, surveys, Astrophysics - Astrophysics of Galaxies},
         year = 2019,
        month = jul,
       volume = {880},
       number = {1},
          eid = {L14},
        pages = {L14},
          doi = {10.3847/2041-8213/ab2c80},
archivePrefix = {arXiv},
       eprint = {1906.11842},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...880L..14C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Schreiber2018b,
       author = {{Schreiber}, C. and {Glazebrook}, K. and {Nanayakkara}, T. and {Kacprzak}, G.~G. and {Labb{\'e}}, I. and {Oesch}, P. and {Yuan}, T. and {Tran}, K. -V. and {Papovich}, C. and {Spitler}, L. and {Straatman}, C.},
        title = "{Near infrared spectroscopy and star-formation histories of 3 {\ensuremath{\leq}} z {\ensuremath{\leq}} 4 quiescent galaxies}",
      journal = {\aap},
     keywords = {techniques: spectroscopic, galaxies: evolution, galaxies: high-redshift, galaxies: statistics, Astrophysics - Astrophysics of Galaxies},
         year = 2018,
        month = oct,
       volume = {618},
          eid = {A85},
        pages = {A85},
          doi = {10.1051/0004-6361/201833070},
archivePrefix = {arXiv},
       eprint = {1807.02523},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018A&A...618A..85S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Popesso2022,
       author = {{Popesso}, P. and {Concas}, A. and {Cresci}, G. and {Belli}, S. and {Rodighiero}, G. and {Inami}, H. and {Dickinson}, M. and {Ilbert}, O. and {Pannella}, M. and {Elbaz}, D.},
        title = "{The Main Sequence of star-forming galaxies across cosmic times}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2022,
        month = mar,
          eid = {arXiv:2203.10487},
        pages = {arXiv:2203.10487},
archivePrefix = {arXiv},
       eprint = {2203.10487},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220310487P},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


