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 />
estimate derived from the spacecraft telemetry and which provides our initial pointing estimate). This<br />
corrected pointing history file (the “superboresight" file) is then applied to the BCD at the pointing<br />
transfer stage <strong>of</strong> the BCD pipeline. The superboresight RA and Dec estimates are recorded in the<br />
CRVAL1 and CRVAL2 FITS keywords, and the position angle estimate is recorded in the CD matrix<br />
keywords. The uncorrected RA and DEC are retained, but called ORIG_RA, ORIG_DEC, as is the<br />
pointing refinement solution for each frame (as RARFND and DECRFND). Note that to use the<br />
superboresight solution, USE REFINED POINTING = 0 should be set in the MOPEX namelists.<br />
Superboresight was implemented as a patch to the S13 s<strong>of</strong>tware build, thus most (but not all) data<br />
processed with S13 or subsequent pipeline versions will have it. Users should check for the presence <strong>of</strong><br />
the ORIG_RA, ORIG_DEC keywords to see if it has been applied to their data. From S14 onwards, the<br />
HDR data have the long frame RA, Dec solution copied to the short frames, as the short frame pointing<br />
solutions are less accurate. Neither superboresight nor pointing refinement are run on the subarray data.<br />
.<br />
5.3.3 Mosaicking and Coaddition<br />
Using the refined coordinates, individual <strong>IRAC</strong> BCDs from a given observation (AOR) are reconstructed<br />
onto a larger field (mosaicking), and overlapping frames are averaged together to achieve a higher S/N.<br />
Outlier rejection is performed on sets <strong>of</strong> overlapping pixels. Because Spitzer observations cover such a<br />
large area, individual BCDs are remapped onto a common grid with a technique similar to “drizzle”<br />
(Fruchter & Hook 2002, [11]). The pixel size in the mosaics produced by the pipeline is exactly 0.6<br />
arcseconds x 0.6 arcseconds in the final data processing. The masks are used in the coaddition in such a<br />
way that the pixels previously flagged as bad (for example, hot or dead pixels) are rejected before the<br />
averaging process. Cosmic rays are rejected at this point via the outlier rejection algorithm. Users will<br />
receive a single coadded image per channel, and per observation (AOR). It will be accompanied by a<br />
coverage map and an uncertainty file per channel per exposure time.<br />
Pipeline Processing 96 Level 2 (Post-BCD) Pipeline