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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

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