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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<strong>IRAC</strong> <strong>Instrument</strong> <strong>Handbook</strong><br />
Again, the “truth image” <strong>of</strong> the background is used to compute a robust weighted DC <strong>of</strong>fset. The banding<br />
artifact is extra flux above the background and it will be subtracted out and saved into the CBCD image.<br />
The<strong>IRAC</strong> pipeline does not model the flaring <strong>of</strong> banding towards the edges <strong>of</strong> the array. Therefore, the<br />
pipeline correction is not always perfect. More information about banding can be found in Section 7.3.2.<br />
5.2.6 Muxstripe Correction (Channels 1 and 2)<br />
For a very bright source, muxbleed is accompanied by a pinstripe pattern (“muxstripe”; every 4 th column<br />
from the bright source is affected) that may extend over part <strong>of</strong> the image preceding or following the<br />
bright pixel (for example, see Figure 7.2 and Figure 7.3). Stars, hot pixels, and particle hits can generate<br />
muxbleed and muxstripe. In the artifact correction pipeline, a procedure was developed to mitigate the<br />
muxstripe in the image.<br />
Figure 5.10. An image showing all four readout channel images side by side. These have been<br />
obtained by rearranging the columns in the original image. Muxbleed is apparent in the bottom<br />
right <strong>of</strong> the 4 th readout channel image.<br />
The algorithm involves converting the BCD image into 256X64 pixel arrays (each <strong>of</strong> the four readout<br />
channels into a separate image; every fourth column is read out by the same channel; see Figure 5.10).<br />
Pipeline Processing 92 The Artifact-Corrected BCD<br />
Pipeline