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 |
muse_std.py
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VERSION |
1.0 -- copied from v. 0.1 when Muse became operational September 2014
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SYNTAX |
PYTHON
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CALL |
processQC
from $DFS_PRODUCT/STD/$DATE
/home/muse/python/muse_std.py -i -a $AB
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INSTRUMENT |
MUSE
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RAWTYPE |
STD
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PURPOSE |
QC check on intermediate (PRO.CATG=PIXTABLE_STD) and master (PRO.CATG=DATACUBE_STD) std frames
check done per CHANEL/IFU (x24) of the PIXTABLE_STD frames
check done also on the combined DATACUBE_STD frame
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PROCINPUT |
PIXTABLE_STD and DATACUBE_STD products
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QC1TABLE |
trending | table(s) in QC1 database:
muse_std
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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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std0.png
left panel: 3D cube collapsed along wavelength direction
righ panel: zoom of the central area of the 3D cube collapsed along wavelength direction
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QC1PARAM |
QC1 parameters written in QC1 database:
QC1 DB names: nsaturated | lambda_shift | pos1_x | pos1_y |
fwhm1_x | fwhm1_y
All parameters are calculated by the pipeline recipe.
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ALGORITHM |
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CERTIF |
Reasons for rejection:
saturation, no target in the FOV
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COMMENTS |
based on original Python script from March 2014
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[2015-11-05T15:00:22] created by qcDocu v1.1.2, a tqs tool
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