QC documentation system: QC procedure xshooter_std_slit_stare.py for XSHOOTER

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] xshooter_bias.py xshooter_dark.py xshooter_dark_nir.py xshooter_detlin.py xshooter_fmtchk.py xshooter_orderdef.py xshooter_wave.py xshooter_flexure.py xshooter_flat_slit.py xshooter_arc_slit.py xshooter_flat_ifu.py xshooter_arc_ifu.py xshooter_std_slit_stare.py xshooter_std_slit_nodoff.py xshooter_sci_slit_stare.py xshooter_sci_slit_nodoff.py xshooter_sci_ifu.py   bottom  plots   |   contact NAME xshooter_std_slit_stare.py VERSION 1.0 -- September 2009 1.1 -- 2017-09-12, docu updated SYNTAX PYTHON CALL processQC from $DFS_PRODUCT/STD_TELL_SLIT_STARE_<arm>/$DATE /home/python/xshooter_std_slit_stare.py -i -a $AB INSTRUMENT XSHOOTER RAWTYPE STD_TELL_SLIT_STARE_NIR | STD_TELL_SLIT_STARE_VIS PURPOSE QC check of processed standard star exposures, extracted spectra, and other products PROCINPUT product standard star frames QC1TABLE trending | table(s) in QC1 database: xshooter_telluric TRENDPLOT trending | HealthCheck plot associated to this procedure: none QC1PAGE trending | associated documentation: standard_qc1.html QC1PLOTS top std_tell_slit_stare_VIS_X00.png extracted merged 1D spectrum with automatic y-axis limits (often useless) std_tell_slit_stare_VIS_X04.png 2D merged spectrum averaged along dispersion axis to get spatial profile std_tell_slit_stare_VIS_A00.png 4-corner display of sky-subtracted STD_TELL_SLIT_STARE_VIS frame std_tell_slit_stare_VIS_A01.png 4-corner display of sky-background fitted to STD_TELL_SLIT_STARE_VIS frame with predicted sky line positions marked std_tell_slit_stare_VIS_A02.png full display of merged 2D STD_TELL_SLIT_STARE_VIS frame std_tell_slit_stare_NIR_X00.png extracted merged 1D spectrum with automatic y-axis limits (often useless) std_tell_slit_stare_NIR_X04.png 2D merged spectrum averaged along dispersion axis to get spatial profile std_tell_slit_stare_NIR_A00.png 4-corner display of sky-subtracted STD_TELL_SLIT_STARE_NIR frame std_tell_slit_stare_NIR_A01.png 4-corner display of sky-background fitted to STD_TELL_SLIT_STARE_NIR frame with predicted sky line positions marked std_tell_slit_stare_NIR_A02.png full display of merged 2D STD_TELL_SLIT_STARE_NIR frame QC1PARAM QC1 parameters written into QC1 table: none QC1db names: flux<i> (i=1...3) | err<i> (i=1...3) | sn<i> (i=1...3) | npix_sat | fpix_sat FITS key names: QC.FLUXi.VAL (i=1...3) | QC.FLUXi.ERR (i=1...3) | QC.FLUXi.SN (i=1...3) | QC.NPIXSAT | QC.FPIXSAT ALGORITHM CERTIF Reasons for rejection: saturated spectra; less than 1000 ADU in continuum for telluric standards in VIS/NIR arm COMMENTS The script is used for STD_FLUX_SLIT_STARE as well, a very rare RAW_TYPE, since flux stds are acquired with the NODDING template Only in the first years flux stds were acquired with the OFFSET template top [2017-11-08T13:19:32]         created by qcDocu v1.1.2, a tqs tool