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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COMMENT 1 blank line<br />
BUNIT = 'MJy/sr ' / Units <strong>of</strong> image data<br />
FLUXCONV= 0.2008 / Flux Conv. factor (MJy/sr per DN/sec)<br />
GAIN = 3.8 / e/DN conversion.<br />
5.1.20 Pointing Transfer (calculation <strong>of</strong> pointing information)<br />
<strong>IRAC</strong> <strong>Instrument</strong> <strong>Handbook</strong><br />
The Pointing Transfer pipeline is a separate script from the actual data reduction pipeline script, designed<br />
to insert raw-pointing and distortion information into the FITS headers <strong>of</strong> BCDs. Like the reduction<br />
pipeline, it executes on a per-BCD basis. Pointing data was acquired by the spacecraft star-tracker at a<br />
rate <strong>of</strong> 2 Hz, transferred to the boresight onboard, and down-linked every 12 hours as a Boresight<br />
Pointing History File (BPHF). The BPHF is received via a separate telemetry stream from the science<br />
data. The first step in pointing transfer is to aquire the portion <strong>of</strong> the BPHF which spans the integration<br />
time <strong>of</strong> the BCD (getPH module). The 2 Hz sampled data are then transferred to the specific channeldependent<br />
science FOV using a set <strong>of</strong> Euler transformations handled by the "BORESIGHTTRAN<br />
module". The Euler angles relating the boresight and FOV positions have been determined in-flight and<br />
are stored in a configuration file.<br />
The pointing samples are then averaged and combined by the "ANGLEAVG" module to compute the<br />
raw-pointing for the BCD: CRVAL1 (RA), CRVAL2 (Dec) and PA (position angle). These, along with<br />
uncertainties and reference pixel coordinates (CRPIX1, CRPIX2), are inserted as keywords into the FITS<br />
header <strong>of</strong> the BCD. The module also computes a CD matrix and transfers distortion coefficients<br />
(represented in the pixel coordinate frame) from a calibration file to the FITS header. The default<br />
projection type for the celestial reference system (CTYPE keyword) is "TAN-SIP". This is a tangent<br />
(TAN) projection modified to make use <strong>of</strong> the Spitzer Imaging (distortion) Polynomials (SIP) in<br />
coordinate mappings.<br />
The Final Product Generator (FPG) is executed at the end. This reformats the FITS header and adds<br />
additional keywords, which are most useful to the user, from the database. An example <strong>of</strong> a BCD header<br />
containing pointing and distortion information is given below.<br />
SIMPLE = T / Fits standard<br />
BITPIX = -32 / FOUR-BYTE SINGLE PRECISION FLOATING POINT<br />
NAXIS = 2 / STANDARD FITS FORMAT<br />
NAXIS1 = 256 / STANDARD FITS FORMAT<br />
NAXIS2 = 256 / STANDARD FITS FORMAT<br />
ORIGIN = 'Spitzer Science Center' / Organization generating this FITS file<br />
CREATOR = 'S18.7.0 ' / SW version used to create this FITS file<br />
TELESCOP= 'Spitzer ' / SPITZER Space Telescope<br />
INSTRUME= '<strong>IRAC</strong> ' / SPITZER Space Telescope instrument ID<br />
/ TARGET AND POINTING INFORMATION<br />
OBJECT = 'NGC7479 ' / Target Name<br />
OBJTYPE = 'TargetFixedSingle' / Object Type<br />
CRPIX1 = 128. / Reference pixel along axis 1<br />
Pipeline Processing 86 Level 1 (BCD) Pipeline