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 |
xshooter_sci_slit_stare.py
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VERSION |
1.0 -- September 2009
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SYNTAX |
PYTHON
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CALL |
processQC
from $DFS_PRODUCT/SCI_SLIT_STARE_<arm>/$DATE
/home/python/xshooter_sci_slit_stare.py -i -a $AB
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INSTRUMENT |
XSHOOTER
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RAWTYPE |
SCI_SLIT_STARE_NIR | SCI_SLIT_STARE_VIS | SCI_SLIT_STARE_UVB
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PURPOSE |
2020-10-01 This script is only used for STD FLUX STARE
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PROCINPUT |
product science frames
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QC1TABLE |
trending | table(s) in QC1 database:
xshooter_sci_slit
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TRENDPLOT |
trending | HealthCheck plot associated to this procedure: none
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QC1PAGE |
trending | associated documentation:
standard_qc1.html
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QC1PLOTS
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sci_slit_nod_VIS_A02.png
full display of merged 2D frame, broken in four parts
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QC1PARAM |
QC1 parameters written into QC1 table: none
QC1db names: flux<i> (i=1...3) | err<i> (i=1...3) | sb<i> (i=1...3) | npix_sat | fpix_sat
FITS key names: QC.FLUXi.VAL (i=1...3) | QC.FLUXi.ERR (i=1...3) | QC.FLUXi.SN (i=1...3) | QC.NPIXSAT | QC.FPIXSAT
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ALGORITHM |
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CERTIF |
Reasons for rejection: saturated spectra
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COMMENTS |
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[2020-10-08T14:13:32] created by qcDocu v1.1.2, a tqs tool
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