IRAC Instrument Handbook - IRSA - California Institute of Technology
IRAC Instrument Handbook - IRSA - California Institute of Technology
IRAC Instrument Handbook - IRSA - California Institute of Technology
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C.1 Use <strong>of</strong> the Five Times Oversampled PRFs Outside <strong>of</strong> APEX<br />
Point Source Fitting <strong>IRAC</strong> Images<br />
with a PRF<br />
154<br />
<strong>IRAC</strong> <strong>Instrument</strong> <strong>Handbook</strong><br />
As supplied in the documentation website, the PRFs are oversampled by a factor <strong>of</strong> five in Delta_x and<br />
Delta_y. This allows for 5x5=25 independent realizations <strong>of</strong> a point source, corresponding to 25 different<br />
pixel phase combinations (five each in x and y). To obtain any given point source realization (PSR), the<br />
PRF needs to be sampled every fifth pixel in x and y at the appropriate phase, i.e.,<br />
PSR1(i,j) = PRF(5i-4,5j-4)<br />
PSR2(i,j) = PRF(5i-4,5j-3)<br />
PSR3(i,j) = PRF(5i-4,5j-2)<br />
PSR4(i,j) = PRF(5i-4,5j-1)<br />
PSR5(i,j) = PRF(5i,5j)<br />
PSR6(i,j) = PRF(5i-3,5j-4)<br />
…………………………….<br />
PSR13(i,j) = PRF(5i-2,5j-2)<br />
PSR25(i,j) = PRF(5i,5j)<br />
where i,j are integers running from 1 to n in the case <strong>of</strong> a PRF table which is 5n x 5n in size. In this case,<br />
PSR13 corresponds to the source landing in the center <strong>of</strong> a pixel. Note that the PRF should not be block<br />
averaged, as this will result in the loss <strong>of</strong> the pixel phase information.<br />
These PRFs may be implemented directly by those willing to write their own code. In IDL, for example, a<br />
point source realization may be generated using the /SAMPLE switch in REBIN, e.g,<br />
psr = rebin(phasedPRF,n,n,/SAMPLE)<br />
where phasedPRF is the 5n x 5n PRF shifted to the appropriate pixel phase in both dimensions. In IRAF,<br />
use:<br />
imcopy PRF.fits[1:5n-4:5,1:5n-4:5] PSR1.fits<br />
Note that the PSRs are normalized to unity at infinity, not to the <strong>IRAC</strong> 10 pixel calibration aperture.<br />
Fluxes obtained with these thus need to be multiplied by the appropriate infinite aperture correction.<br />
These have been determined to be 0.943 in channel 1 and 0.929 in channel 2, based on measurements <strong>of</strong><br />
the PRF, and can be compared to "direct" measurements <strong>of</strong> 0.944 and 0.937. Estimates from the PRF are<br />
unavailable in channels 3 and 4, but the corrections given in this <strong>Handbook</strong> are 0.772 and 0.737,<br />
respectively (Table 4.7).<br />
C.2 Modifications to the <strong>IRAC</strong> PRFs for Use with APEX