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_WAVE.sh
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VERSION |
1.0 -- 2015-04-01 begin of operations
1.1 -- 2017-09-05 docu updated
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SYNTAX |
SHELL
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CALL |
called by processQC from $DFS_PRODUCT/IFS_WAVE/$DATE as
qc_IFS_WAVE -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_WAVE
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PURPOSE |
quality control script for SPHERE IFS WAVE pipeline products
level 0 : writeQC scoreQC.
level 1 : calls qc_mstplt.py -a $AB
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PROCINPUT |
-a AB -level level
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QC1TABLE |
trending | table(s) in QC1 database:
sphere_ifs_wave
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_IFS_DISP_HC.html |
trend_report_IFS_RESPOW_HC.html
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QC1PAGE |
trending | associated documentation:
SP_IFS_wave_qc1.html
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QC1PLOTS
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r.SPHER.2017-09-01T14:00:01.904_tpl_X00.png
standard cross sections and raw image zoom
r.SPHER.2017-12-19T10:01:12.257_tpl_0002.png
Arc line spectrum and Gaussian fit results from QC script
r.SPHER.2017-12-19T10:01:12.257_tpl_0003.png
DeltaLambda versus Lambda, dispersion error from QC script
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QC1PARAM |
QC1 parameters written into QC1 table:
QC.LAMP.FLUX.AVG, qc_lamp_flux, lamp
QC.LAMP.FLUX.VARIANCE, qc_lamp_var, rms of lamp
QC.NUM.OUT.OF.DISP, qc_numoutofdisp, (not documented)
QC.BAD.SPECTRA, qc_numbadspec, number of bad spectra
QC.MEDIAN.RESOLVING.POWER, qc_resol_power, resolving power
QC.MEDIAN.DISPERSION, qc_med_dispers, dispersion
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ALGORITHM |
Description of algorithms:
see pipeline user manual.
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CERTIF |
Reasons for rejections: lamp is off
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COMMENTS |
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[2017-12-22T12:30:39] created by qcDocu v1.1.2, a tqs tool
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