QC documentation system: QC procedure xshooter_sci_ifu.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_sci_ifu.py VERSION 1.0 -- September 2009 1.1 -- June 2010 SYNTAX PYTHON CALL processQC from $DFS_PRODUCT//$DATE /home/python/xshooter_sci_ifu_off.py -i -a $AB INSTRUMENT XSHOOTER RAWTYPE SCI_IFU_OFF_NIR | SCI_IFU_OFF_VIS | SCI_IFU_OFF_UVB | STD_FLUX_IFU_OFF_NIR | STD_FLUX_IFU_OFF_VIS | STD_FLUX_IFU_OFF_UVB SCI_IFU_STARE_NIR | SCI_IFU_STARE_VIS | SCI_IFU_STARE_UVB | STD_FLUX_IFU_STARE_NIR | STD_FLUX_IFU_STARE_VIS | STD_FLUX_IFU_STARE_UVB STD_TELL_IFU_STARE_NIR | STD_TELL_IFU_STARE_VIS | STD_TELL_IFU_STARE_UVB | STD_TELL_IFU_STARE_NIR | STD_TELL_IFU_STARE_VIS | STD_TELL_IFU_STARE_UVB PURPOSE QC check of processed standard star or science exposures PROCINPUT product standard star or science frames QC1TABLE trending | table in QC1 database: none TRENDPLOT trending | HealthCheck plot associated to this procedure: none QC1PAGE trending | associated documentation: night_ifu_qc1.html QC1PLOTS top sci_ifu_offset_UVB_X00.png differences of traces in slice 1-2, 2-3, 1-3 vs wavelength sci_ifu_offset_UVB_X01.png differences of traces in slice 1-2, 2-3, 1-3 vs wavelength (blow-up) sci_ifu_offset_UVB_A00.png XY plane of cube sci_ifu_offset_UVB_A01.png YZ plane of cube sci_ifu_offset_UVB_A02.png XZ plane of cube sci_ifu_offset_VIS_X00.png differences of traces in slice 1-2, 2-3, 1-3 vs wavelength sci_ifu_offset_VIS_X01.png differences of traces in slice 1-2, 2-3, 1-3 vs wavelength (blow-up) sci_ifu_offset_VIS_A00.png XY plane of cube sci_ifu_offset_VIS_A01.png YZ plane of cube sci_ifu_offset_VIS_A02.png XZ plane of cube sci_ifu_offset_NIR_X00.png differences of traces in slice 1-2, 2-3, 1-3 vs wavelength sci_ifu_offset_NIR_X01.png differences of traces in slice 1-2, 2-3, 1-3 vs wavelength (blow-up) sci_ifu_offset_NIR_A00.png XY plane of cube sci_ifu_offset_NIR_A01.png YZ plane of cube sci_ifu_offset_NIR_A02.png XZ plane of cube QC1PARAM QC1db names: avg<ij> (ij=12/23/13) | rms<ij> (ij=12/23/13) | med<ij> (ij=12/23/13) FITS key names: QC.TRACEij.AVG (ij=12/23/13) | QC.TRACEij.RMS (ij=12/23/13) | QC.TRACEij.MED (ij=12/23/13) QC1db names: min<ij> (ij=12/23/13) | max<ij> (ij=12/23/13) | npix_sat | fpix_sat FITS key names: QC.TRACEij.MIN (ij=12/23/13) | QC.TRACEij.MAX (ij=12/23/13) | QC.NPIXSAT | QC.FPIXSAT ALGORITHM CERTIF Reasons for rejection: saturated spectra (traces may be very noisy for faint targets) COMMENTS top [2017-11-08T13:20:00]         created by qcDocu v1.1.2, a tqs tool