QC documentation system: QC procedure xshooter_flat_slit.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   ESPRESSO   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_flat_slit.py VERSION : 1.0 -- February 2009 : 1.1 -- 2017-09-01 docu updated for slit function and flat spectrum plots SYNTAX PYTHON CALL processQC from $DFS_PRODUCT/FLAT_SLIT_<arm>/$DATE: $DFO_PROC_DIR/python/xshooter_flat_slit.py -i -a $AB INSTRUMENT XSHOOTER RAWTYPE FLAT_SLIT_UVB | FLAT_SLIT_VIS | FLAT_SLIT_NIR PURPOSE compares product FLAT_SLIT_<arm> files for XSHOOTER QC assessment; the plots are later reviewed within certifyProducts. The plot is stored in $DFO_PLT_DIR. PROCINPUT master FLAT_SLIT and fitted background QC1TABLE trending | table(s) in QC1 database: xshooter_flat TRENDPLOT trending | HealthCheck plot(s) associated to this procedure: trend_report_FLAT_SLIT_UVB_HC.html | trend_report_FLAT_SLIT_VIS_HC.html | trend_report_FLAT_SLIT_NIR_HC.html QC1PAGE trending | associated documentation: flat_qc1.html QC1PLOTS top flat_slit_UVB_A00.png full display of master FLAT_SLIT_UVB frame with fitted order edge positions overplotted flat_slit_UVB_A01.png enlargements of the edge regions of master FLAT_SLIT_UVB frame with fitted order edge positions overplotted flat_slit_UVB_A02.png full display of background fitted to FLAT_SLIT_UVB frame with fitted order edge positions overplotted flat_slit_UVB_A03.png full display of master FLAT_SLIT_UVB frame divided by reference frame flat_slit_UVB_A05.png cross section of selected order and linear fit to slit function illumination gradient flat_slit_UVB_013.png D2 lamp, black: master flat spectrum, red: reference spectrum, magenta: ratio spectrum and linear least square fit, green aligned master flat, blue: residuals flat_slit_UVB_014.png QTH lamp, black: master flat spectrum, red: reference spectrum, magenta: ratio spectrum and linear least square fit, green aligned master flat, blue: residuals flat_slit_UVB_015.png D2+QTH lamp, black: master flat spectrum, red: reference spectrum, magenta: ratio spectrum and linear least square fit, green aligned master flat, blue: residuals flat_slit_VIS_A00.png full display of master FLAT_SLIT_VIS frame with fitted order edge positions overplotted flat_slit_VIS_A01.png enlargements of the edge regions of master FLAT_SLIT_VIS frame with fitted order edge positions overplotted flat_slit_VIS_A02.png full display of background fitted to FLAT_SLIT_VIS frame with fitted order edge positions overplotted flat_slit_VIS_A03.png full display of master FLAT_SLIT_VIS frame divided by reference frame flat_slit_VIS_A05.png cross section of selected order and linear fit to slit function illumination gradient flat_slit_VIS_013.png black: master flat spectrum, red: reference spectrum, magenta: ratio spectrum and linear least square fit, green aligned master flat, blue: residuals flat_slit_NIR_A00.png full display of master FLAT_SLIT_NIR frame with fitted order edge positions overplotted flat_slit_NIR_A01.png enlargements of the edge regions of master FLAT_SLIT_NIR frame with fitetd order positions overplotted flat_slit_NIR_A02.png full display of background fitted to FLAT_SLIT_NIR frame with fitted order edge positions overplotted flat_slit_NIR_A03.png full display of master FLAT_SLIT_NIR frame divided by reference frame flat_slit_NIR_A05.png cross section of selected order and linear fit to slit function illumination gradient flat_slit_NIR_013.png black: master flat spectrum, red: reference spectrum, magenta: ratio spectrum and linear least square fit, green aligned master flat, blue: residuals QC1PARAM QC1 parameters written into QC1 table (UVB has 2 separate lamps): QC1db names: min_flux_1 | max_flux_1 | max_flux_norm_1 FITS key names: QC.FLUX.MIN | QC.FLUX.MAX | flux_norm_1 QC1db names: (only UVB, QTH lamp) min_flux_2 | max_flux_2 | max_flux_norm_2 FITS key names: QC.FLUX.MIN | QC.FLUX.MAX | flux_norm_2 QC1 params created by pipeline: all except flux_norm_1/2 (= max_flux_1/2 divided by exposure time) ALGORITHM CERTIF Reasons for rejection: - saturation or severe underexposure; for UVB: lack of one lamp COMMENTS In case a new flat field lamp is inserted in the instrument: 1) edit $DFO_CONFIG_DIR/trendPlotter/lamp_exchange_list.txt 2) call $DFO_CONFIG_DIR/trendPlotter/lamp_exchange_run.sh to update LAMP_EXCHANGE_QTH.py (and others) to be called by HC plot to mark dates of lamp exchange by blue bars top [2021-03-05T21:05:09]         created by qcDocu v1.1.2, a tqs tool