QC documentation system: QC procedure pionier_speccalQC.py for PIONIER

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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pionier_badpix.py pionier_darkQC.py pionier_kappaQC.py pionier_speccalQC.py
pionier_OIFITS_fringeQC.py pionier_OIFITS_intfringeQC.py
 
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NAME pionier_speccalQC.py
VERSION 1.0 -- 2015-06-06
SYNTAX PYTHON
CALL measureQuality
from $DFS_PRODUCT/SPECTRAL_CALIBRATION/$DATE:
 pionier_speccalQC.py -a $AB
INSTRUMENT PIONIER
RAWTYPE RAW_SPEC_CALIBRATION
PURPOSE a) generates QC reports
PROCINPUT No special input is required:
a) $DATE is read from the input AB
c) frames are implicitly read from the AB.
QC1TABLE trending | table(s) in QC1 database:
pionier_spec_calibration
TRENDPLOT trending | HealthCheck plot(s) associated to this procedure:
trend_report_SPECTRAL_CALIB_HC.html
QC1PAGE trending | associated documentation:
speccal_qc1.html
QC1PLOTS
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r.PIONI.2015-11-28T09:05:00.033_tpl_0000.png

r.PIONI.2015-11-28T09:05:00.033_tpl_0001.png

r.PIONI.2015-11-28T09:05:00.033_tpl_0002.png

r.PIONI.2015-11-28T09:05:00.033_tpl_0003.png
QC1PARAM QC1 parameters written into QC1 table :
SOURCE(header/script)       DBNAME                 value          description

 QC.EFFWAVE	spec_cal_effwave  1.6e-6 	effective central wave
 QC.EFFBAND	spec_cal_effband  4.32e-8 	effective band
 QC.EFFWAVE.PTP	spec_cal_effwave_ptp  4.3e-8	effective central wave variation between the baselines (peak to peak)
ALGORITHM Description of algorithms:
This measures the effective wavelength of each spectral channel
by measuring the actual fringes spacing for long scans.
This is only possible if the internal piezo scanner is well calibrated/known and linear
Data can be taken on sky (used to calibrate sky data).
or on the internal lamp (HC).
using the Fourier Transform Spectrometry of the fringes
CERTIF Products are rejected if the central wavelength is too far off
Products are rejected if the effective band is too far off
COMMENTS None
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