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 |
pionier_darkQC.py
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VERSION |
1.0 -- 2015-06-06
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SYNTAX |
PYTHON
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CALL |
measureQuality from $DFS_PRODUCT/DARK_CALIBRATION/$DATE:
pionier_darkQC.py -a $AB
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INSTRUMENT |
PIONIER
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RAWTYPE |
RAW_DARK_CALIBRATION
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PURPOSE |
a) generates QC reports
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PROCINPUT |
No special input is required:
a) $DATE is read from the input AB
c) frames are implicitly read from the AB.
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QC1TABLE |
trending | table(s) in QC1 database:
pionier_dark
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_DARK_HC.html
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QC1PAGE |
trending | associated documentation:
det_qc1.html
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QC1PLOTS
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r.PIONI.2015-11-28T09:04:20.747_0000.png
r.PIONI.2015-11-28T09:04:20.747_0001.png
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QC1PARAM |
QC1 parameters written into QC1 table :
SOURCE(header/script) DBNAME value description
QC.DARK.MED dark_median 28 dark_in_adu
QC.DARKRMS.MAX dark_rms_max 5.4 max_error_of_dark_in_adu
QC.DARKRMS.MED dark_rms_med 1.03 median_error_of_dark_in_adu
QC.NOISE.MED dark_noise_med 20.3 median_of_noise_in_adu
QC.NOISE.MAX dark_noise_max 61.9 max_of_nois_in_adu
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ALGORITHM |
Description of algorithms:
The detector behaviors are characterized by measuring the dark level
and the power spectral density.
data are taken with all shutters closed
Data can be taken on sky (used to calibrate sky data).
or on the internal lamp (HC).
Compute the DARK signal as an average over the scan
The DARK value should be stable over the scan : average all points of the scan
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CERTIF |
Products are rejected only if issue with detector
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COMMENTS |
None
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[2016-11-02T07:22:48] created by qcDocu v1.1.2, a tqs tool
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