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 |
vimos_stdmos.py
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VERSION |
1.0 -- July 2010 to February 2011
1.0.1 -- skip call of scoreQC (2011-05-31)
1.0.2 -- histogram of raw frame added (2012-01-17)
1.0.3 -- QC1 parameters num_overexp/level_overexp added (2012-01-20)
1.0.4 -- changes needed for muc (2013-02-07)
1.0.5 -- changes for qc_imadisp v1.5 (2014-01-20)
1.0.6 -- remove usage of has_key dictionary attribute (2014-03-12)
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SYNTAX |
PYTHON
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CALL |
processQC
from $DFS_PRODUCT/STD_MOS/$DATE
/home/vimos/python/vimos_stdmos.py -i -a $AB
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INSTRUMENT |
VIMOS
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RAWTYPE |
STD_MOS
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PURPOSE |
QC check of pipeline products from MOS standard stars
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PROCINPUT |
products: MOS_SPECPHOT_TABLE, OBJ_STD_TABLE, MOS_STANDARD_SKY
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QC1TABLE |
trending | table(s) in QC1 database:
vimos_mos_std
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_MOSEFF_LRb_HC.html
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QC1PAGE |
trending | associated documentation:
mos_stdeff_qc1.html
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QC1PLOTS
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stdmos1.png
upper left panel: extracted spectrum of standard and error spectrum
middle left panel: extracted sky spectrum (complete view)
lower left panel: extracted sky spectrum around selected sky lines
upper right panel: histogram of raw frame
middle right panel: efficiency spectra for all four quadrants
(per wavelength bin and interpolated)
lower right panel: current response curve compared to master response
stdmos2.png
MOS_STANDARD SKY: this is the sky that is subtracted from the slit spectra
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QC1PARAM |
QC1 parameters written in QC1 database: efficiency1 | efficiency2 | ... | efficiency15
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ALGORITHM |
Description of algorithms:
efficiencyNN: ratio of the detected number of photons to the real number of photons
at dedicated wavelength ranges
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CERTIF |
Reasons for rejection:
strongly deviating fluxes between quadrants, very low efficiencies
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COMMENTS |
NONE
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[2016-03-11T12:31:23] created by qcDocu v1.1.2, a tqs tool
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