| 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_STD_SPEC.sh
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| 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)
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| SYNTAX |
SHELL
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| CALL |
processQC
from $DFS_PRODUCT/STD_SPEC/$DATE:
qc_STD_SPEC $date $primfile "
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| INSTRUMENT |
VISIR
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| RAWTYPE |
STD_SPEC
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| 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
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| PROCINPUT |
spectroscopic standard star product
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| QC1TABLE |
trending | table(s) in QC1 database:
visir_zp_spc
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| TRENDPLOT |
trending | HealthCheck plot associated to this procedure: none
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| QC1PAGE |
trending | associated documentation: none
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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
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| ALGORITHM |
Description of algorithms:
For details see VISIR Pipeline User Manual
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| CERTIF |
Reasons for rejection: spectrum too faint
Reasons for rejection: detector artifacts too bright
Frame is displayed to check for unusual patterns, artificial structures
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| COMMENTS |
NONE
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[2012-06-20T10:57:07] created by qcDocu v1.1.2, a tqs tool
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