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 |
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VERSION |
1.0 -- December 2009
1.0.1 -- supporting numpy V1.3 and matplotlib V0.99 (2010-02-08)
1.0.2 -- overplots Balmer series (2011-02-28)
1.0.3 -- skip call of scoreQC (2011-05-31)
1.0.4 -- QC1 parameters num_overexp/level_overexp added (2012-01-20)
1.0.5 -- for new HR_blue grisms (2012-06-05)
1.0.6 -- bug fix with plot for all four quadrants (2012-07-09)
1.0.7 -- changes needed for muc (2013-02-07)
1.0.8 -- remove usage of has_key dictionary attribute (2014-03-12)
1.1 -- new: plot response curve (2014-06-06)
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SYNTAX |
PYTHON
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CALL |
processQC
from $DFS_PRODUCT/STD_IFU/$DATE
/home/vimos/python/vimos_stdifu.py -i -a $AB
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INSTRUMENT |
VIMOS
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RAWTYPE |
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PURPOSE |
QC check on IFU standard star products
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PROCINPUT |
products: IFU_SCIENCE_SKY, IFU_STD_FOV, IFU_SPECPHOT_TABLE
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QC1TABLE |
trending | table(s) in QC1 database:
vimos_ifu_std
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_IFUEFF_LRb_HC.html |
trend_report_IFUEFF_LRr_HC.html |
trend_report_IFUEFF_MR_HC.html |
trend_report_IFUEFF_HRb_HC.html |
trend_report_IFUEFF_HRo_HC.html |
trend_report_IFUEFF_HRr_HC.html
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QC1PAGE |
trending | associated documentation:
ifu_stdeff_qc1.html
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QC1PLOTS
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stdifu0.png
upper left panel: extracted and summed up object spectrum
middle left panel: sky spectrum
lower left panel: details of sky spectrum with comparison to nominal wavelengths
of sky lines
upper right panel: efficiency vs. wavelength for all 4 quadrants;
they are plotted per wavelength bin and as a smoothed and interpolated version
middel right panel: current response curve compared to master response
lower right panel: reconstructed field of view; combined image for all 4 quadrants
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QC1PARAM |
QC1 parameters written in QC1 database: efficiency1 | efficiency2 | ... | efficiency15
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ALGORITHM |
Description of algorithms:
efficiencyNN: ratio of the detected number of photons to the real number of photons
at dedicated wavelength ranges
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CERTIF |
Reasons for rejection:
observation without attached (mandatory) calibrations,
badly reconstructed IFU image,
low flux because of instrumental problems or unstable weather conditions
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COMMENTS |
NONE
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[2016-03-11T12:31:27] created by qcDocu v1.1.2, a tqs tool
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