Index A ACS channels ACS electronics failure Jan. 2007 analog-to-digital (A-to-D) conversion 1, 2 aperture correction apertures HRC and WFC in V2/V3 frame WFC in V2/V3 frame archive association tables astrometry absolute ACS coordinate transformations impact of guide star failures relative aXe 1, 2 B bad pixels data quality flags bias jumps bias subtraction C calacs 1, 2 acs2d 1, 2 acsccd 1, 2 acsrej (cosmic ray rejection task) acssum calibration steps calibration switch selection criteria doAtoD (A-to-D correction) doBias (bias image subtraction) doBlev (bias level correction, overscan subtraction) doDark (dark image subtraction) doDQI (bad pixel determination) 1, 2 doFlash (post-flash subtraction) doFlat (flat field image correction) doNoise (initialize error array) 1, 2 doNonLin (linearity correction, MAMA data) doPhot (photometry keywords calculation) doShad (shutter shading correction) doStat (image statistics determination) gain correction processing and combining sub-exposures processing dithered exposures processing single exposures processing speed product file suffixes trailer files calibration A-to-D errors bias errors calacs flat fields gain manual recalibration photometry polarimetry 1, 2 ramp filters readout noise shading correction spectroscopy Calibration Database System (CDBS) CCD bias jumps CTE full well depth hot and warm pixels hot columns HRC bias level determination linearity linearity beyond saturation post-SM4 sub-array bias gradient post-SM4 WFC bias gradient post-SM4 WFC bias striping post-SM4 WFC signal-dependent bias shift quantization noise readout noise saturation sub-arrays WFC bias level determination charge diffusion charge transfer efficiency (CTE) charge diffusion HRC HRC CTE equation image anomalies internal measurements pixel-based CTE corrections 1, 2 trend and evolution WFC WFC equation coronagraphy flat fields ghosts photometry PSF subtraction cosmic ray rejection cosmic rays D dark current features increasing rate reference file (DARKFILE) data array size (pixels) associations calibrated and drizzled formats file definitions file size (MB) files and suffixes FITS file structure multi-extension FITS storage and transfer storage requirements trailer files units for calacs files units for calibrated data units for drizzled data units for raw data Data Archive and Distribution System (DADS) data quality array initialization bad pixel flags detector apertures in V2/V3 frame characteristics orientation F filter wheel position accuracy FITS files flat fields CCD ground flats CCD L-flats correction coronagraphy Earth flats pipeline flats pixel area map polarimetry SBC ground flats SBC L-flats correction sky flats flat-fielded images (flt.fits) photometry G gain calibration correction in calacs (doFlat) Generic Conversion geometric distortion pixel area map grism guide star failures H hot pixels annealing growth HRC coronagraphic flats coronagraphic photometry coronagraphic PSF subtraction CTE 1, 2 CTE equation Earth flats linearity linearity beyond saturation ramp filters red leak UV contamination UV PSF I icons used in this manual image anomalies charge transfer efficiency (CTE) cross-talk dust motes optical ghosts scattered Earth light scattered light image header keywords extension header keywords group header keywords primary header keywords image units 1, 2, 3 M MAMA linearity correction MultiDrizzle memory requirements units O observing strategies On-The-Fly Reprocessing (OTFR) system Operations Pipeline Unified System (OPUS) optical design P parallel operations performance after SM4 sub-array bias gradient WFC bias gradient WFC bias striping WFC signal-dependent bias shift photometry ABMAG aperture correction bypassing PHOTCORR step during recalibration color correction coronagraphy header photometric systems pixel area map red leaks reference files header keywords STMAG UV contamination VEGAMAG zeropoints pipeline Calibration Database System (CDBS) Generic Conversion On-The-Fly Reprocessing (OTFR) Operations Pipeline Unified System (OPUS) processing steps PyDrizzle pixel area map (PAM) point spread function (PSF) as a function of source color coronagraphic PSF subtraction field dependence long wavelength artifacts Tiny Tim UV polarimetry calibration 1, 2 diattenuation flat field geometric distortion instrumental issues phase retardance zeropoint 1, 2 post-calibration WFC bias stripe removal prism PyDrizzle R ramp filters apertures ground calibration recalibration setting switches skipping doPhot step red leaks HRC SBC reference files A-to-D correction table (ATODTAB) bias image (BIASFILE) calibration switches CCD characteristics table (CCDTAB) cosmic ray rejection table (CRREJTAB) dark image (DARKFILE) 1, 2 flat field image (PFLTFILE, LFLTFILE, DFLTFILE, CFLTFILE) header keywords MAMA linearity table (MLINTAB) overscan table (OSCNTAB) permanent bad pixels (BPIXTAB) 1, 2 post-flash image (FLSHFILE) shutter shading image (SHADFILE) throughput component tables (GRAPHTAB, COMPTAB) S saturation CCD linearity SBC dark countrate red leaks UV contamination UV PSF shutter stability South Atlantic Anomaly (SAA) spectroscopy AUTOIMAGE background bright stars calibration crowding data reduction with aXe dithering extra field objects flat fielding flux calibration resolution wavelength calibration zeroth order T target acquisitions Tiny Tim typographic conventions in this manual 1, 2 U units for images 1, 2 UV contamination W warm pixels warning types in this document WFC CTE 1, 2 CTE equation linearity linearity beyond saturation ramp filters sky flats Z zeropoints