QC documentation system: QC procedure muse_throughput.py for MUSE

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 MIDI PIONIER   OMEGACAM VIRCAM [best viewing with style sheets and javascript enabled] muse_bias.py muse_dark.py muse_lampflat.py muse_skyflat.py muse_arc.py muse_throughput.py muse_std.py muse_astrometry.py   bottom  plots   |   contact NAME muse_throughput.py VERSION 1.0 -- copied from v. 0.1 when Muse became operational September 2014 SYNTAX PYTHON CALL processQC from $DFS_PRODUCT/STD/$DATE /home/muse/python/muse_throughput.py -i -a $AB INSTRUMENT MUSE RAWTYPE THROUGHPUT PURPOSE QC check on MASTER_AMPL product check done per CHANEL/IFU (x24) qc parameters extracted from TABLE_AMPL master product PROCINPUT MASTER_AMPL and TABLE_AMPL products QC1TABLE trending | table(s) in QC1 database: muse_throughput TRENDPLOT trending | HealthCheck plot associated to this procedure: none QC1PAGE trending | associated documentation: none QC1PLOTS top throughput0.png snapshot of all the detectors QC1PARAM QC1 parameters written in QC1 database: QC1 DB names: thru1 | thru2 | thru2_err | slice_thru2 | photons | power All parameters are calculated by the pipeline recipe. ALGORITHM CERTIF Reasons for rejection: NONE, technical calibration COMMENTS based on original Python script from March 2014 top [2015-11-05T15:00:19]         created by qcDocu v1.1.2, a tqs tool