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 |
vimos_scimos.py
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VERSION |
1.0 -- June 2010 to February 2011
1.0.1 -- create cover sheet (2011-05-27)
1.0.2 -- skip call of scoreQC (2011-05-31)
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SYNTAX |
PYTHON
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CALL |
processQC
from $DFS_PRODUCT/STD_IFU/$DATE
/home/vimos/python/vimos_scimos.py -i -a $AB
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INSTRUMENT |
VIMOS
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RAWTYPE |
SCI_MOS
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PURPOSE |
QC check of MOS science products
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PROCINPUT |
products: MOS_SCIENCE_REDUCED, MOS_SCIENCE_EXTRACTED, OBJECT_SCI_TABLE, MOS_SCIENCE_SKY
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QC1TABLE |
trending | table(s) in QC1 database:
vimos_mos_sci
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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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scimos1.png
extracted spectra and error spectra for three objects
scimos2.png
upper panel: extracted sky spectra belonging to three different objects (complete view)
lower panel: extracted sky spectra around selected sky lines
scimos3.png
This plot can be produced up to four times for LR and two times for MR grisms
depending on the number of multiplex layers.
left panel: extracted and calibrated sky spectra per slit
right panel: extracted and calibrated sky spectra per slit (detail)
scimos4.png
This plot can be produced up to four times for LR and two times for MR grisms
depending on the number of multiplex layers.
left panel: extracted and calibrated slit spectra, sky subtracted
right panel: extracted and calibrated slit spectra
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QC1PARAM |
QC1 parameters written in QC1 database: ids_rms | deltatime_std
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ALGORITHM |
Description of algorithms:
ids_rms: rms of dispersion solution, taken from calibration
deltatime_std: time difference to standard star exposure
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CERTIF |
Reasons for notes in GEN_INFO/NOTES.txt:
not well wavelength-calibrated, i.e. skylines at wrong positions
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COMMENTS |
NONE
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[2016-03-11T12:31:31] created by qcDocu v1.1.2, a tqs tool
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