QC documentation system: QC procedure run_kappa.csh for MIDI

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   VIRCAM [best viewing with style sheets and javascript enabled] run_detron.csh run_detlin.csh run_dettrn.csh run_refpix.csh run_wave.csh run_kappa.csh run_data_quality_processQC.csh extractVis_dispersed.csh extractTF_dispersed.csh extractbinned_dispersed.csh plot_data_dispersed.csh midi_frg_hs_disp_display.csh midi_frg_sp_disp_display.csh   bottom  plots   |   contact NAME run_kappa.csh VERSION 1.0 SYNTAX SHELL CALL processQC -a abname or . $DFO_PROC_DIR/run_data_quality_processQC.csh $RAW_TYPE $DATE $PF . $DFO_PROC_DIR/run_kappa.csh INSTRUMENT MIDI RAWTYPE CAL_SP_KAPPA PURPOSE extracting values of the KAPPA_MATRIX PROCINPUT products under CAL_SP_KAPPA QC1TABLE trending | table(s) in QC1 database: midi_kappa TRENDPLOT trending | HealthCheck plot(s) associated to this procedure: trend_report_KAPPA_HC.html | trend_report_KAPPA_GRISM_HC.html QC1PAGE trending | associated documentation: MIDI_QC_tutorial_kappa.html QC1PLOTS top trend_report_KAPPA_HC.png value of the median and stddev for the kappa matrix (SCI_PHOT mode) QC1PARAM QC1 parameters written into QC1 table: QC1db names: midi_kappa FITS key names: QC.KAPPA.MEDIAN11/12/21/22 | QC.KAPPA.STDDEV11/12/21/22 QC1 params created by pipeline: all QC1 params created by this procedure: none ALGORITHM Description of algorithms: The kappa coefficients are measured using the photometric files taken with an SCI_PHOT observation. The photometry files associated to the SCI_PJHOT observation (if requested by the PI) could be used to calibrate the fringes taken in SCI_PHOT mode. For now we use a static kappa matrix (calculated accumulating 6 months or more of data) to calibrate the fringes. This is only used for instrument monitoring. CERTIF (guidelines for acceptance/rejection)Should be within a certain threshold (see HC plots). If the object is too faint, there are some problems COMMENTS MIDI is misaligned in reference with the VLTI beam, this causes the k22 to be overestimated top [2011-10-19T09:32:23]         created by qcDocu v1.1.2, a tqs tool