QC documentation system: QC procedure qc_IFS_SPOS 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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NAME qc_IFS_SPOS.sh
VERSION 1.0 -- 2015-04-01 begin of operations
1.1 -- 2017-09-05 docu updated
SYNTAX SHELL
CALL called by processQC
from $DFS_PRODUCT/IFS_SPOS/$DATE as
qc_IFS_SPOS -a $AB -level 1 2\>\&1 \> $DFS_LOG/$AB.qclog
meaning output is logged to $DFS_LOG/$AB.qclog !!!
INSTRUMENT SPHERE
RAWTYPE IFS_SPOS
PURPOSE quality control script for SPHERE IFS spectral positions pipeline products
level 0 : debug, implicit call of writeQC scoreQC.
level 1 : calls qc_mstplt.py -a $AB
PROCINPUT -a AB -level level
QC1TABLE trending | table(s) in QC1 database:
sphere_ifs_specpos
TRENDPLOT trending | HealthCheck plot(s) associated to this procedure:
trend_report_IFS_SPOS_YJ_HC.html | trend_report_IFS_SPOS_YJH_HC.html | ../../../ALL/ref_frames/ref_sphere.html
QC1PAGE trending | associated documentation:
SP_IFS_spos_qc1.html
QC1PLOTS
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r.SPHER.2015-03-23T09:14:54.836_tpl_X00.png
standard cross sections and image zoom
QC1PARAM QC1 parameters written into QC1 table:
QC.NUMBER.SPECTRA, qc_number_spectra, number of used spectra
QC.SCALE.MEASURED qc_scale_measured, correcting scale
DRS.OFFSETX.MEASURED, qc_offset_x, offset applied to transformation
DRS.OFFSETY.MEASURED, qc_offset_y, offset applied to transformation
DRS.IFS.MAX.LAMBDA, qc_max_lambda
DRS.IFS.MIN.LAMBDA, qc_min_lambda
DRS.IFS.DISPERSION dispersion
DRS.DIST.X/Y.COEFF.0/3_0/3, qc_dist_x/y_0/3_0/3, polynomial coefficients for optical disrotion correction
ALGORITHM Description of algorithms:
see pipeline user manual
CERTIF Reasons for rejection
COMMENTS the lamp counts are not monitored
top [2017-12-22T12:30:38]         created by qcDocu v1.1.2, a tqs tool