QC documentation system: QC procedure muse_astrometry.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_dark.py VERSION 1.0 -- copied from v. 0.1 when Muse became operational September 2014 SYNTAX PYTHON CALL processQC from $DFS_PRODUCT/ASTROMETRY/$DATE /home/muse/python/muse_std.py -i -a $AB INSTRUMENT MUSE RAWTYPE ASTROMETRY PURPOSE QC check on intermediate (PRO.CATG=PIXTABLE_ASTROMETRY) and master (PRO.CATG=DATACUBE_ASTROMETRY) std frames check done per CHANEL/IFU (x24) of the PIXTABLE_ASTROMETRY frames check done also on the combined DATACUBE_ASTROMETRY frame PROCINPUT PIXTABLE_ASTROMETRY and DATACUBE_ASTROMETRY products QC1TABLE trending | table(s) in QC1 database: muse_std TRENDPLOT trending | HealthCheck plot associated to this procedure: none QC1PAGE trending | associated documentation: none QC1PLOTS top astrometry0.png left panel: 3D cube collapsed along wavelength direction righ panel: zoom of the central area of the 3D cube collapsed along wavelength direction QC1PARAM QC1 parameters written in QC1 database: QC1 DB names: nsaturated | lambda_shift | nstars | medres_x | medres_y scale_x | scale_y |angle_x | angle_y All parameters are calculated by the pipeline recipe. ALGORITHM CERTIF Reasons for rejection: saturation, no target in the FOV, bad astrometric solution/fit COMMENTS based on original Python script from March 2014 top [2015-11-05T15:03:33]         created by qcDocu v1.1.2, a tqs tool