QC documentation system: QC procedure qc_ILLU for ISAAC

This documentation is intended both for QC scientists and SciOps astronomers (who may want to ignore the technical information displayed in grey).   HOME   CRIRES FORS2   FORS1 GIRAFFE UVES XSHOOTER   ISAAC VIMOS VISIR   HAWKI NACO SINFONI   AMBER MIDI   OMEGACAM VIRCAM [best viewing with style sheets and javascript enabled] qc_DARK qc_CHECK_FLAT qc_IMG_FLAT qc_SP_FLAT qc_ZPOINT qc_TELLURIC qc_SP_ARC qc_STARTRACE qc_SLIT qc_ILLU qc_LINE qc_SCI_IMG qc_SCI_SPEC   bottom  plots   |   contact NAME qc_ILLU.sh VERSION 1.0 -- 2006-07-27 fill template by handbook 1.2 -- 2007-12-11 updated in frame of QC tutorial migration 1.3 -- 2008-01-09 bug in trending plots (../FULL included) 1.4 -- 2008-04-21 writeQC replaces get_QC1 and call_qc1_illu SYNTAX SHELL CALL processQC from $DFS_PRODUCT/ILLU/$DATE: qc_LINE -d $DATE -f $primfile INSTRUMENT ISAAC RAWTYPE ILLU PURPOSE writes QC1 parameters into local list PROCINPUT a) $DATE in yyyy-mm-dd, b) $primfile is the PRO.CATG=ILLUM_FRAME product with the _0000.fits extension. c) raw frames are implicitely read from the AB. QC1TABLE trending | table(s) in QC1 database: isaac_illu TRENDPLOT trending | HealthCheck plot(s) associated to this procedure: ../FULL/trend_report_EFFILL_SJ_HC.html QC1PAGE trending | associated documentation: qc_IS_illum.html QC1PLOTS top illu0.png illumination product QC1PARAM FITSNAME, DBNAME , typical value, description: QC.ILLUM1 , qc_illum1, illumination fit coefficient QC.ILLUMX , qc_illumx, lllumination fit coefficient QC.ILLUMY , qc_illumy, illumination fit coefficient QC.ILLUMXX , qc_illumxx, illumination fit coefficient QC.ILLUMYY , qc_illumyy, illumination fit coefficient QC.ILLUMXY , qc_illumxy, illumination fit coefficient ---------- , qc_eff_ul, illumination correction in center of ul quadrant ---------- , qc_eff_ur, illumination correction in center of ur quadrant ---------- , qc_eff_ll, illumination correction in center of ll quadrant ---------- , qc_eff_lr, illumination correction in center of lr quadrant ---------- , qc_eff_cc, illumination correction in center of detector ---------- , qc_corr_mean, mean of 5 effective correction values ---------- , qc_corr_stdev, rms of 5 effective correction values ---------- , qc_flux_mean, mean of 17 flux values ---------- , qc_flux_stdev, rms of 17 flux values ---------- , qc_x1 , position of source in first frame ---------- , qc_y1 , position of source in first frnme ---------- , qc_f1 , flux of source in first frame ALGORITHM Description of algorithms: Fits a 2-degree polynomial to the 9 measurements of the photometric standard star distributed over thew FOV CERTIF NONE COMMENTS illumination frames have been reprocessed in 2007-10, There is a document about this. The star is rtied to be identified by the QC script and the star name, RA, DEC, V and MK are written into the DB as well top [2012-06-20T10:57:32]         created by qcDocu v1.1.2, a tqs tool