QC documentation system: QC procedure qc_IFS_DFLAT for SPHERE

This documentation is intended both for QC scientists and SciOps astronomers (who may want to ignore the technical information displayed in grey).
 
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qc_IRD_DARK qc_IRD_BACK qc_IRD_FLAT qc_IRD_DIST
qc_IFS_DARK qc_IFS_BACK qc_IFS_DFLAT qc_IFS_SPOS qc_IFS_WAVE qc_IFS_FLAT qc_IFS_DIST
qc_ZPL_BIAS_IMG qc_ZPL_BIAS_POL qc_ZPL_DARK_IMG qc_ZPL_DARK_POL qc_ZPL_IFLAT_IMG qc_ZPL_IFLAT_POL qc_ZPL_MODEM_EFF
 
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NAME qc_IFS_DFLAT.sh
VERSION 1.0 -- 2015-04-01 begin of operations
1.1 -- 2017-09-05 docu updated
SYNTAX SHELL
CALL called by processQC
from $DFS_PRODUCT/IFS_DFLAT/$DATE as
qc_IFS_DFLAT -a $AB -u vircam -level 1 2\>\&1 \> $DFS_LOG/$AB.qclog
meaning output is logged to $DFS_LOG/$AB.qclog !!!
INSTRUMENT SPHERE
RAWTYPE IFS_DFLAT
PURPOSE quality control script for SPHERE IFS imaging flats pipeline products
level 0 : debug, implicit call of writeQC scoreQC.
level 1 : calls gen_pipe_suppl_histofit_I.py -a $AB -e $extension
level 1 : calls gen_pipe_raw_stat_IV.py -a $AB -e $extension
PROCINPUT -a AB -level level
QC1TABLE trending | table(s) in QC1 database:
sphere_ifs_dflat
TRENDPLOT trending | HealthCheck plot(s) associated to this procedure:
trend_report_IFS_DFLAT_YJ_HC.html | trend_report_IFS_DFLAT_YJH_HC.html | trend_report_IFS_DFLAT_NBP_YJ_HC.html | trend_report_IFS_DFLAT_NBP_YJH_HC.html
QC1PAGE trending | associated documentation:
SP_IFS_dflat_qc1.html
QC1PLOTS
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r.SPHER.2017-09-01T13:23:14.491_tpl_0010.png
two raw frame cubes, each cube with 10 layers
32 pre-amplifier channels and their relative gain.
QC1PARAM QC1 parameters written into QC1 table:
QC.LAMP.FLUX.AVG.2, qc_lam_flux_avg_0 first raw frame counts
QC.LAMP.FLUX.AVG.7 qc_lam_flux_avg_1 second raw frame counts
QC.PREAMP.CORR.MEDIAN15 qc_preamp_med_1 pre-amplifier of channel #15
QC.FPN qc_fpn fixed pattern noise (normalized)
QC.FLAT.NONLINEARITY qc_flat_nonlin non-linearity
ALGORITHM Description of algorithms:
See pipeline user manual
CERTIF Reasons to reject:
unexposed or saturated
COMMENTS The IFS imaging flats (called detector flats by the pipeline) come for both prisms and for five different lamps, four narrow band laser lamps (lamps 1-4) and one broad band halogen lamp (lamp5). The pre-amplier map product is generated only for the broad band halogen lamp flat.
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