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_IFS_DARK.sh
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VERSION |
1.0 -- 2015-04-01
1.1 -- 2017-09-05 docu updated
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SYNTAX |
SHELL
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CALL |
called by processQC from $DFS_PRODUCT/IFS_DARK/$DATE as
qc_IFS_DARK -a $AB -u sphere -level 1 2\>\&1 \> $DFS_LOG/$AB.qclog
meaning output is logged to $DFS_LOG/$AB.qclog !!!
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INSTRUMENT |
SPHERE
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RAWTYPE |
IFS_DARK
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PURPOSE |
quality control script for SPHERE IFS DARK pipeline products
level 0 : debug case, only inplicit call of writeQC scoreQC.
level 1 : calls ${HOME}/python/qc_mstplt.py -a $AB
and calls ${HOME}/progs/gen_pipe_suppl_raw_I.py -a $AB
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PROCINPUT |
-a $AB -u sphere -level 1
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QC1TABLE |
trending | table(s) in QC1 database:
sphere_ifs_dark
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_IFS_DARK_med_HC.html |
trend_report_IFS_DARK_ron_HC.html |
trend_report_IFS_DARK_HP_HC.html |
../../../ALL/ref_frames/ref_sphere.html
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QC1PAGE |
trending | associated documentation:
SP_IFS_dark_qc1.html
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QC1PLOTS
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r.SPHER.2017-08-31T10:29:33.401_tpl_0010.png
one raw frame. dark values for each plane of the raw cube
r.SPHER.2017-08-31T10:29:33.401_tpl_X00.png
standard cross sections
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QC1PARAM |
QC1 parameters written into QC1 table:
QC.MEDIANMASTER, qc_med median dark level
QCRON (LOCAL), qc_ron from QC script
QC.NUM.HOTPIXELS, qc_num_hotpix number of hot pixel
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ALGORITHM |
Description of algorithms:
For each pixel the stddev is calulated from plane 11-15 from the raw input cube.
The median of all stdev is called qc_ron.
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CERTIF |
Reasons for rejection:
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COMMENTS |
The dark current and the ron is increasing with exposure time.
The persistence vanished in dark frames from 2017-05-10 on
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[2017-12-22T12:30:33] created by qcDocu v1.1.2, a tqs tool
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