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 |
crires_dark.py
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VERSION |
1.0 -- October 2013
1.0.1 -- usage of qc_mstplt v1.4 instead of kmos_mstplt (2014-01-15)
1.0.2 -- usage of argparse module (2014-03-07)
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SYNTAX |
PYTHON
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CALL |
processQC
from $DFS_PRODUCT/DARK/$DATE
/home/python/kmos_dark.py -i -a $AB
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INSTRUMENT |
KMOS
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RAWTYPE |
DARK
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PURPOSE |
QC check of raw and product dark exposures
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PROCINPUT |
raw, product, and reference dark frames
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QC1TABLE |
trending | table(s) in QC1 database:
kmos_dark
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_DARKLEV_HC.html |
trend_report_DARKRON_HC.html
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QC1PAGE |
trending | associated documentation:
dark_qc1.html
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QC1PLOTS
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dark1.png
top: current master dark for detectors 1, 2, and 3
bottom: current master dark - master reference dark; detectors 1, 2, and 3
dark2.png
top: central area of current master dark for detectors 1, 2, and 3
bottom: current master dark - master reference dark (central area); detectors 1, 2, and 3
dark3.png
upper left: cuts in X direction through master and raw frames
upper middle: cuts in Y direction through master and raw frames
upper right: histograms of first raw frame and master
central left: cuts in X direction through master and raw frames, central area
central middle: cuts in Y direction through master and raw frames, central area
central right: row and column averages of master
lower left: master - reference frame, cut in X direction
lower middle: master - reference frame, cut in Y direction
lower right: histogram of master - reference frame
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QC1PARAM |
QC1 parameters written in QC1 database:
QC1 DB names: dark_mean | dark_median | ron_mean | ron_median | dark_current | badpix
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ALGORITHM |
dark_mean: mean of master dark [ADU]
dark_median: median of master dark [ADU]
ron_mean: mean noise of master dark [ADU]
ron_median: median noise of master dark [ADU]
dark_current: dark current [e-/s]
badpix: number of bad pixels
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CERTIF |
KMOS darks frequently show remnants from previous exposures.
Frames with unusual high dark values and/or an unusual structure should be rejected.
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COMMENTS |
None
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[2015-10-29T10:46:55] created by qcDocu v1.1.2, a tqs tool
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