QC documentation system: QC procedure qc_STD_SPEC.sh for VISIR

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_DARK_IMG.sh qc_DARK_SPEC.sh
qc_FF_IMG.sh qc_FF_IMG_TECH.sh qc_FF_SPEC.sh qc_FF_SPEC_TECH.sh
qc_STD_IMG.sh qc_STD_SPEC.sh qc_STD_ECH.sh
qc_SCI_IMG.sh qc_SCI_SPEC.sh
 
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NAME qc_STD_SPEC.sh
VERSION 1.0 -- created (2005-03-07)
1.1 -- QC parameters extracted from headers of products (2005-11-07)
1.2 -- extended the list of QC parameters (2006-09-26)
SYNTAX SHELL
CALL processQC
from $DFS_PRODUCT/STD_SPEC/$DATE:
qc_STD_SPEC $date $primfile "
INSTRUMENT VISIR
RAWTYPE STD_SPEC
PURPOSE extracts QC parameters and records them in the local qclog table $DFO_TREND_DIR/STD_SPEC.qclog and in qc1 database table visir_zp_spc
PROCINPUT spectroscopic standard star product
QC1TABLE trending | table(s) in QC1 database:
visir_zp_spc
TRENDPLOT trending | HealthCheck plot associated to this procedure: none
QC1PAGE trending | associated documentation: none
QC1PLOTS
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QC1PARAM QC1 parameters written into QC1 table: sens_mean/stdev | backgd_mean | xcshift
QC1 parameters written into local QC1 table $DFO_TREND_DIR/STD_SPEC.qclog:
QC.SENS.MEAN | QC.SENS.STDEV | QC.BACKGD.MEAN
QC.SENSIT.MEAN: - computed in units mJy at 10sigma in 1 houry; it's average across whole spectrum
FITS key names: INS.PFOV | DET.DIT | FILTER2 | INS.RESOL | INS.GRAT1.WLEN | GRAT1 | INS.SLIT1.WID | AIRMASS
QC1 params created by pipeline: all
QC1 params created by this procedure: none
ALGORITHM Description of algorithms:
For details see VISIR Pipeline User Manual
CERTIF Reasons for rejection: spectrum too faint
Reasons for rejection: detector artifacts too bright
Frame is displayed to check for unusual patterns, artificial structures
COMMENTS NONE
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