QC documentation system: QC procedure xshooter_arc_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_arc_ifu.py VERSION : 1.0 -- February 2009 SYNTAX PYTHON CALL processQC from $DFS_PRODUCT/ARC_IFU_<arm>/$DATE: $DFO_PROC_DIR/python/xshooter_arc_ifu.py -i -a $AB INSTRUMENT XSHOOTER RAWTYPE ARC_IFU_UVB | ARC_IFU_VIS | ARC_IFU_NIR PURPOSE compares raw and product ARC_IFU_<arm> files for XSHOOTER QC assessment; the plots are later reviewed within certifyProducts. The plot is stored in $DFO_PLT_DIR. PROCINPUT pre-processed ARC_IFU; residual table; QC1TABLE trending | table(s) in QC1 database: xshooter_wavecal TRENDPLOT trending | HealthCheck plot(s) associated to this procedure: trend_report_ARC_IFU_time_UVB_HC.html | trend_report_ARC_IFU_time_VIS_HC.html | trend_report_ARC_IFU_time_NIR_HC.html QC1PAGE trending | associated documentation: wavecal_qc1.html QC1PLOTS top arc_ifu_UVB_X00.png top left:: resolution vs. line tilt top right:: resolution vs. wavelength bottom:: shift vs. wavelength arc_ifu_UVB_A00.png full display of pre-processed ARC_IFU_UVB frame with identified lines overplotted arc_ifu_UVB_A01.png enlargements of the edge regions of pre-processed ARC_IFU_UVB frame with identified lines overplotted arc_ifu_VIS_X00.png top left:: resolution vs. line tilt top right:: resolution vs. wavelength bottom:: shift vs. wavelength arc_ifu_VIS_A00.png full display of pre-processed ARC_IFU_VIS frame with identified lines overplotted arc_ifu_VIS_A01.png enlargements of the edge regions of pre-processed ARC_IFU_VIS frame with identified lines overplotted arc_ifu_NIR_X00.png top left:: resolution vs. line tilt top right:: resolution vs. wavelength bottom:: shift vs. wavelength arc_ifu_NIR_A00.png full display of pre-processed ARC_IFU_NIR frame with identified lines overplotted arc_ifu_NIR_A01.png enlargements of the edge regions of pre-processed ARC_IFU_NIR frame with identified lines overplotted QC1PARAM QC1 parameters written into QC1 table: QC1db names: npix_sat | fpix_sat | line_intensity | resold-med | resol_rms | fwhm | fwhm_rms FITS key names: QC.NPIXSAT | QC.FPIXSAT |QC.NLININT | QC.RESOLMED | QC.RESOLRMS | QC.WAVECAL.FWHM.SPACE | QC.FWHMRMS QC1db names: nline_found | nline_cat | model_diffy_avg | model_diffy_med | model_diffy_rms FITS key names: QC.WAVECAL.FOUNDLINE | QC.WAVECAL.CATLINE | QC.MODEL.WAVECAL.DIFFYAVG | QC.MODEL.WAVECAL.DIFFYMED | QC.MODEL.WAVECAL.DIFFYSTD QC1 params created by pipeline: all ALGORITHM CERTIF Reasons for rejection: - no lines - strong slope of shift vs wavelength (indicates ADC problems for VIS) COMMENTS top [2017-11-08T13:19:29]         created by qcDocu v1.1.2, a tqs tool