QC documentation system: QC procedure espre_ledff.py for ESPRESSO

This documentation is intended both for QC scientists and SciOps astronomers (who may want to ignore the technical information displayed in grey).   HOME   CRIRES FORS1 FORS2 KMOS NACO   GIRAFFE UVES XSHOOTER   ISAAC SPHERE VIMOS VISIR   HAWKI MUSE SINFONI   AMBER GRAVITY MIDI PIONIER   OMEGACAM VIRCAM [best viewing with style sheets and javascript enabled] espre_bias.py espre_dark.py espre_ledff.py espre_orderdef.py espre_flat.py espre_wave.py   bottom  plots   |   contact NAME espre_ledff.py VERSION 1.0 -- Ocotober 2018 1.0.1 -- fix max counts QC parameter (2018-11-07) SYNTAX PYTHON CALL processQC from $DFS_PRODUCT/LED_FF/$DATE /home/python/espre_ledff.py -i -a $AB INSTRUMENT ESPRESSO RAWTYPE LED_FF PURPOSE QC check of raw and product LED FF exposures PROCINPUT raw and product LED FF frames QC1TABLE trending | table(s) in QC1 database: espresso_ledff TRENDPLOT trending | HealthCheck plot(s) associated to this procedure: trend_report_BADPIX_HR1x1_HC.html | trend_report_CONAD_HR1x1_HC.html QC1PAGE trending | associated documentation: ledff_qc1.html QC1PLOTS top ledff1.png One plot for BLUE and one for RED raw frames. upper left: cuts in X direction through first and last raw frame upper middle: cuts in Y direction through first and last raw frame upper right: histograms of first and last raw frame left: cuts in X direction, central area middle: cuts in Y direction, central area right: 2D image of first raw frame QC1PARAM QC1 parameters written in QC1 database: QC1 DB names: badpix_nb_avg | badpix_nb_rms | badpix_nb_tot | gain_avg | gain_rms | counts_min_avg | counts_min_rms | counts_max_avg | counts_max_rms ALGORITHM Pipeline QC parameter come per read-out port. The QC script calculates the average and the RMS across the ports plus the total number of bad pixels. CERTIF The frames with highest exposure time should not be saturated. COMMENTS None top [2020-09-01T15:26:22]         created by qcDocu v1.1.2, a tqs tool