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; $Id: extract_stars.pro, v 1.1 Mar 2012 e.d. $
; $Id: extract_stars.pro, v 2.0 Sep 2024 e.d. $
;
;+
; NAME:
......@@ -26,11 +26,24 @@
; MODIFICATION HISTORY:
; Written by: Emiliano Diolaiti, June 2001.
; 1) Created this file (E. D., March 2012).
; 2) Modified data type: from array of structures to structure of arrays (E.D., September 2024).
;-
FUNCTION extract_stars, list, n
on_error, 2
s = where_stars(list, n)
if n ne 0 then return, list[s] else return, -1
if n ne 0 then begin
sublist = starlist(n)
sublist.x = list.x[s]
sublist.sigma_x = list.sigma_x[s]
sublist.y = list.y[s]
sublist.sigma_y = list.sigma_y[s]
sublist.f = list.f[s]
sublist.sigma_f = list.sigma_f[s]
sublist.c = list.c[s]
sublist.is_a_star = list.is_a_star[s]
endif else $
sublist = -1
return, sublist
end
; $Id: is_star.pro, v 1.0 Sep 2024 e.d. $
;
;+
; NAME:
; IS_STAR
;
; PURPOSE:
; Check status of one or more elements in the list of stars and presumed stars.
;
; CATEGORY:
; STARFINDER auxiliary procedures.
;
; CALLING SEQUENCE:
; Result = IS_STAR(List, S)
;
; INPUTS:
; List: list of stars and presumed stars
;
; S: subscript(s) of element(s) to be checked
;
; OUTPUTS:
; Return scalar or array of binary values for each element defined by parameter S.
; Returned value is 1 for a confirmed star, 0 otherwise.
;
; MODIFICATION HISTORY:
; Written by: Emiliano Diolaiti, September 2024.
;-
FUNCTION is_star, list, s
on_error, 2
return, list.is_a_star[s] and 1B
end
; $Id: merge_list.pro, v 1.1 Mar 2001 e.d. $
; $Id: merge_list.pro, v 2.0 Sep 2024 e.d. $
;
;+
; NAME:
......@@ -23,6 +23,7 @@
; Written by: Emiliano Diolaiti, June 2001.
; 1) Created this file (E. D., March 2012).
; 2) Fixed bug when input list L1 is empty (E. D., April 2012).
; 3) Modified data type: from array of structures to structure of arrays (E.D., September 2024).
;-
FUNCTION merge_list, l1, l2
......@@ -31,13 +32,17 @@ FUNCTION merge_list, l1, l2
if n_tags(l1) eq 0 then $
l = l2 else $
begin
n1 = n_elements(l1)
; if n1 eq 0 then l = l2 else $
; begin
n2 = n_elements(l2)
n1 = n_elements(l1.is_a_star)
n2 = n_elements(l2.is_a_star)
l = starlist(n1 + n2)
l[0] = l1 & l[n1] = l2
; endelse
l.x = [l1.x, l2.x]
l.sigma_x = [l1.sigma_x, l2.sigma_x]
l.y = [l1.y, l2.y]
l.sigma_y = [l1.sigma_y, l2.sigma_y]
l.f = [l1.f, l2.f]
l.sigma_f = [l1.sigma_f, l2.sigma_f]
l.c = [l1.c, l2.c]
l.is_a_star = [l1.is_a_star, l2.is_a_star]
endelse
return, l
end
; $Id: reverse_class.pro, v 1.1 Mar 2012 e.d. $
; $Id: reverse_class.pro, v 2.0 Sep 2024 e.d. $
;
;+
; NAME:
......@@ -22,19 +22,19 @@
; of all elements in the list
;
; OUTPUTS:
; Return list where the classification of the subscripted elements;
; is reversed
; Return list where the classification of the subscripted elements is reversed
;
; MODIFICATION HISTORY:
; Written by: Emiliano Diolaiti, June 2001.
; 1) Created this file (E.D., March 2012).
; 2) Modified data type: from array of structures to structure of arrays (E.D., September 2024).
;-
FUNCTION reverse_class, list, SUBSCRIPTS = s
on_error, 2
if n_elements(s) eq 0 then s = lindgen(n_elements(list))
if n_elements(s) eq 0 then s = lindgen(n_elements(list.is_a_star))
l = list
l[s].is_a_star = (not l[s].is_a_star) and 1B
l.is_a_star[s] = (not l.is_a_star[s]) and 1B
return, l
end
; $Id: sort_list.pro, v 1.1 Mar 2012 e.d. $
; $Id: sort_list.pro, v 2.0 Sep 2024 e.d. $
;
;+
; NAME:
......@@ -16,16 +16,15 @@
; INPUTS:
; List: list of stars
;
; KEYWORD PARAMETERS:
; SUBSCRIPTS: subscripts of stars to be sorted. If undefined, sort
; all stars in the list
;
; OUTPUTS:
; Return sorted list of sublist, if SUBSCRIPTS is set.
; OPTIONAL OUTPUTS:
; SUBSCRIPTS: subscripts of sorted stars in the input list.
;
; MODIFICATION HISTORY:
; Written by: Emiliano Diolaiti, June 2001.
; 1) Created this file (E. D., March 2012).
; 2) Modified data type: from array of structures to structure of arrays (E.D., September 2024).
; 3) Corrected comment about keyword parameter SUBSCRIPT
; (it is an optional output, not an optional input) (E.D., September 2024).
;-
FUNCTION sort_list, list, SUBSCRIPTS = s
......@@ -33,5 +32,13 @@ FUNCTION sort_list, list, SUBSCRIPTS = s
on_error, 2
if n_tags(list) eq 0 then return, list
s = reverse(sort(list.f))
return, list[s]
list.x = list.x[s]
list.sigma_x = list.sigma_x[s]
list.y = list.y[s]
list.sigma_y = list.sigma_y[s]
list.f = list.f[s]
list.sigma_f = list.sigma_f[s]
list.c = list.c[s]
list.is_a_star = list.is_a_star[s]
return, list
end
; $Id: star_param.pro, v 1.1 Mar 2012 e.d. $
; $Id: star_param.pro, v 2.0 Sep 2024 e.d. $
;
;+
; NAME:
......@@ -34,6 +34,7 @@
; MODIFICATION HISTORY:
; Written by: Emiliano Diolaiti, June 2001.
; 1) Created this file (E. D., March 2012).
; 2) Modified data type: from array of structures to structure of arrays (E.D., September 2024).
;-
PRO star_param, list, SUBSCRIPTS = s, $
......@@ -45,13 +46,13 @@ PRO star_param, list, SUBSCRIPTS = s, $
endif
n = n_elements(s)
if n eq 0 then begin
n = n_elements(list) & s = lindgen(n) ; extract all elements
n = n_elements(list.is_a_star) & s = lindgen(n) ; extract all elements
endif
if s[0] lt 0 then n = 0 else begin $
x = list[s].x & sigma_x = list[s].sigma_x
y = list[s].y & sigma_y = list[s].sigma_y
f = list[s].f & sigma_f = list[s].sigma_f
c = list[s].c
x = list.x[s] & sigma_x = list.sigma_x[s]
y = list.y[s] & sigma_y = list.sigma_y[s]
f = list.f[s] & sigma_f = list.sigma_f[s]
c = list.c[s]
endelse
return
end
; $Id: starfinder.pro, v 1.8.2a May 2014 e.d. $
; $Id: starfinder.pro, v 1.8.2b_dev01 Sep 2024 e.d. $
;
;+
; NAME:
......@@ -435,6 +435,8 @@
; 26) Removed bug in STARFINDER_FIT module: sometimes very close sources
; were swapped by call to COMPARE_LISTS (E.D., April 2012).
; 27) Updated documentation (E. D., May 2014).
; 28) Modified data type of variable "list_of_stars":
; from array of structures to structure of arrays (E.D., September 2024).
;-
......@@ -1164,7 +1166,9 @@ PRO starfinder, $
; print, "STARFINDER: final re-fitting: iteration", iter + 1
for n = 0L, n_stars - 1 do $
; modified March 2012
if list_of_stars[n].is_a_star or re_fitting eq 1 then $ ;;; if list_of_stars[n].is_a_star or re_fitting eq 1 or iter eq 0 then $
; if list_of_stars[n].is_a_star or re_fitting eq 1 then $ ;;; if list_of_stars[n].is_a_star or re_fitting eq 1 or iter eq 0 then $
; modified September 2024
if is_star(list_of_stars, n) or re_fitting eq 1 then $ ;;; if list_of_stars[n].is_a_star or re_fitting eq 1 or iter eq 0 then $
starfinder_fit, list_of_stars, n, image, siz, background, stars, $
noise_std, sv_par, x_bad, y_bad, fit_par, fit_data, $
model_data, threshold_n, re_fitting, _EXTRA = extra, $
......
; $Id: starlist.pro, v 1.1 Mar 2012 e.d. $
; $Id: starlist.pro, v 2.0 Sep 2024 e.d. $
;
;+
; NAME:
; STARLIST
;
; PURPOSE:
; Create a new list of elements representing either
; true or presumed stars.
; Create a new list of elements representing true or presumed stars.
;
; CATEGORY:
; STARFINDER auxiliary procedures.
......@@ -18,24 +17,31 @@
; N: number of elements in the list
;
; OPTIONAL INPUTS:
; X, Y, F: 1D vectors with position and flux of new elements
; X, Y: 1D vectors with positions of new elements
;
; C: 1D vector with correlation coefficients of new elements (if available)
; F: 1D vector with fluxes of new elements (used only if X, Y are defined)
;
; C: 1D vector with correlation coefficients of new elements (used only if X, Y, F are defined)
;
; OUTPUTS:
; Return possibly initialized list of N elements
; Return initialized list of N elements
;
; MODIFICATION HISTORY:
; Written by: Emiliano Diolaiti, June 2001.
; 1) Added optional input C in STARLIST (E.D., March 2012).
; 2) Created this file (E. D., March 2012).
; 2) Created this file (E.D., March 2012).
; 3) Modified data type: from array of structures to structure of arrays (E.D., September 2024).
;-
FUNCTION starlist, n, x, y, f, c
on_error, 2
element = star()
list = replicate(element, n)
list = { $
x: fltarr(n), sigma_x: fltarr(n), $ ; x- coordinate and error
y: fltarr(n), sigma_y: fltarr(n), $ ; y- coordinate and error
f: fltarr(n), sigma_f: fltarr(n), $ ; flux and error
c: make_array(n, VALUE = -1.0), $ ; correlation coefficient
is_a_star: bytarr(n)} ; flag
if n_elements(x) ne 0 and n_elements(y) ne 0 then $
update_list, list, x, y, f, c
return, list
......
; $Id: update_list.pro, v 1.1 Mar 2012 e.d. $
; $Id: update_list.pro, v 2.0 Sep 2024 e.d. $
;
;+
; NAME:
......@@ -25,10 +25,10 @@
; Sigma_X, Sigma_Y, Sigma_F: errors on position and flux.
;
; KEYWORD PARAMETERS:
; SUBSCRIPTS: 1D vector of subscripts of stars to update. If not defined,
; update all the stars in the list.;
; SUBSCRIPTS: 1D vector of subscripts of stars to be updated. If not defined,
; update all the stars in the list.
;
; IS_STAR: set this keyword to say that the stars to update have already
; IS_STAR: set this keyword to specify that the elements to be updated have already
; been accepted as true stars.
;
; OUTPUTS:
......@@ -36,23 +36,24 @@
;
; MODIFICATION HISTORY:
; Written by: Emiliano Diolaiti, June 2001.
; 1) Created this file (E. D., March 2012).
; 1) Created this file (E.D., March 2012).
; 2) Modified data type: from array of structures to structure of arrays (E.D., September 2024).
;-
PRO update_list, list, SUBSCRIPTS = s, x, y, f, c, $
sigma_x, sigma_y, sigma_f, IS_STAR = is_star
sigma_x, sigma_y, sigma_f, IS_STAR = is_star
on_error, 2
n = n_elements(s)
if n eq 0 then s = lindgen(n_elements(x))
if s[0] ge 0 then begin
list[s].x = x & list[s].y = y
if n_elements(f) ne 0 then list[s].f = f
if n_elements(c) ne 0 then list[s].c = c
if n_elements(sigma_x) ne 0 then list[s].sigma_x = sigma_x
if n_elements(sigma_y) ne 0 then list[s].sigma_y = sigma_y
if n_elements(sigma_f) ne 0 then list[s].sigma_f = sigma_f
list[s].is_a_star = keyword_set(is_star) and 1B
list.x[s] = x & list.y[s] = y
if n_elements(f) ne 0 then list.f[s] = f
if n_elements(c) ne 0 then list.c[s] = c
if n_elements(sigma_x) ne 0 then list.sigma_x[s] = sigma_x
if n_elements(sigma_y) ne 0 then list.sigma_y[s] = sigma_y
if n_elements(sigma_f) ne 0 then list.sigma_f[s] = sigma_f
list.is_a_star[s] = keyword_set(is_star) and 1B
endif
return
end