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 |
run_amber_p2vm_qcDocu.csh
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VERSION |
1.0
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SYNTAX |
SHELL
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CALL |
processQC -a abname or
. ~/Isabelle/SCRIPTS/MeasureQuality/run_amber_processQC.sh.averaged $RAW_TYPE $DATE $PF
. ~/Isabelle/SCRIPTS/MeasureQuality/run_amber_p2vm_qcDocu.sh
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INSTRUMENT |
AMBER
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RAWTYPE |
3P2V
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PURPOSE |
extracting various QC parameters
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PROCINPUT |
products under 3P2V
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QC1TABLE |
trending | table(s) in QC1 database:
amber_p2vm
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_P2VM_LJHK_HC.html
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QC1PAGE |
trending | associated documentation:
AMBER_QC_tutorial_p2vm.html
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QC1PLOTS
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trend_report_P2VM_LJHK_HC.png
internal instrumental Visibility (should be stable and as close as possible to 1)
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QC1PARAM |
QC1 parameters written into QC1 table:
QC1db names: amber_p2vm
FITS key names for P2VM: QC.P1/2/3.OFFSETX/Y | QC.P2VM.K/H/J.VIS12/VIS23/VIS31 | QC.P2VM.K/H/J.ERRVIS12/ERRVIS23/ERRVIS31
QC1 params created by pipeline: all
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ALGORITHM |
Description of algorithms:
P2VM: Calculate the internal instrumental Visibility for the different instrumental settings (Low, Medium and High resolution) and for the 3 baselines (12, 23, 31).
The Spectral Configuration is given by OCS.OBS.SPECCONF or INS.MODE, the observing band by QC.BAND. When observing in Low Resolution JHK or Medium Resolution the offsets between the different photometric channels is also measured
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CERTIF |
(guidelines for acceptance/rejection): check if it is within the same range as the HC plots. Should be between .7 and 1 depending of the configuration
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COMMENTS |
(any comments)
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[2010-01-26T09:03:52] created by qcDocu v1.1.2, a tqs tool
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