@@ -224,7 +224,7 @@ is designed to compensate for the gravitational deformations of the whole surfac
<td>beam waveguide</td>
<td>2.7’</td>
<td>32-37(*)</td>
<td>0.60</td>
<td>0.66 (*)</td>
</tr>
<trclass="row-odd"><td>K</td>
<td>18 – 26</td>
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@@ -233,12 +233,12 @@ is designed to compensate for the gravitational deformations of the whole surfac
<td>Gregorian</td>
<td>0.8’(**)</td>
<td>90(**)</td>
<td>0.45-0.65</td>
<td>[0.66]</td>
</tr>
</tbody>
</table>
<p>[ ] is an estimate
(*) at the band’s central frequency
(*) at the band’s central frequency (for C-band: 45 degrees EL @ 7.3 GHz)
(**) at 22.3 GHz with opacity 0.1 and ground air temperature of 293K.</p>
<p>The FWHM beam size, as a function of the frequency f, can be approximated by the following rule: FWHM(arcmin)=19.7/ f(GHz)</p>
<p>SRT receiver changes are quick, allowing for an efficient frequency agility. The selected receiver is set in its focal position within at most a few minutes.
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@@ -558,7 +558,7 @@ Available configurations consist of:</p>
<p><strong>in L band:</strong></p>
<p>The full bandwidth for this receiver is 500 MHz (1.3-1.8 GHz). RF filters can be used (XXL4, XXL2 etc.) as well as additional backend filters (115, 230 or 460 MHz).</p>
<p>More detailed information on the SARDARA backend can be found here: <aclass="reference external"href="https://www.worldscientific.com/doi/full/10.1142/S2251171718500046">SARDARA</a>.</p>
<p>Note: for spectroscopic observations in L-band with SARDARA, only total intensity is offered.</p>
<p>Note: for spectroscopic observations in L-band with SARDARA (with the 115 MHz filter), only total intensity is offered.</p>