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_arc.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 $DFS_PRODUCT/ARC/$DATE
/home/muse/python/muse_arc.py -i -a $AB
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INSTRUMENT |
MUSE
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RAWTYPE |
ARC
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PURPOSE |
QC check on raw and master arc frames
check done per CHANEL/IFU (x24) and slice (x48) of the raw and master arc frames
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PROCINPUT |
raw arc frames and WAVECAL_TABLE product
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QC1TABLE |
trending | table(s) in QC1 database:
muse_wave
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_ARC_wavecal_HC.html |
trend_report_ARC_fit_HC.html
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QC1PAGE |
trending | associated documentation:
wave_qc1.html
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QC1PLOTS
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arc0.png
snapshot of all detectors
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QC1PARAM |
QC1 parameters written in QC1 database:
QC1 DB names: slice1/../48_fit_nlines | slice1/../48_fit_rms | slice1/../48_lines_fwhm_mean |
slice1/../48_resol | slice1/../48_wlen | slice1/../48_wlpos
All parameters are calculated by the pipeline recipe
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ALGORITHM |
Description of algorithms:
slice1/../48_fit_nlines: Number of arc lines used in calibration solution fit in slice
slice1/../48_lines_nid: Number of identified arc lines per slice
slice1/../48_resol: Mean spectral resolution R determined in slice
slice1/../48_wlen: Wavelength associated to WLPOS in slice
slice1/../48_wlpos: Wavelength associated to WLPOS in slice
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CERTIF |
Reasons for rejection:
too small number of arc lines used in wavelength solution, bad fit
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COMMENTS |
based on original Python script from March 2014
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[2015-11-05T15:00:17] created by qcDocu v1.1.2, a tqs tool
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