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 |
kmos_wave.py
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VERSION |
1.0 -- October 2013
1.0.1 -- usage of funtion get_keyval (2013-12-11)
1.0.2 -- create all 2D plots only on demand, option --all (2014-01-10)
1.0.3 -- usage of qc_imaovw instead of kmos_mstovw (2014-01-28)
1.0.4 -- usage of argparse module (2014-03-07)
1.0.5 -- count number of failures of wavelength solution (2014-03-24)
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SYNTAX |
PYTHON
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CALL |
processQC
from $DFS_PRODUCT/WAVE/$DATE
/home/python/kmos_wave.py -i -a $AB
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INSTRUMENT |
KMOS
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RAWTYPE |
WAVE
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PURPOSE |
QC check of raw and product arc-lamp exposures
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PROCINPUT |
raw and product arc-lamp frames
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QC1TABLE |
trending | table(s) in QC1 database:
kmos_wave
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_FWHM_Ar_IZ_HC.html |
trend_report_FWHM_Ar_YJ_HC.html |
trend_report_FWHM_Ar_H_HC.html |
trend_report_FWHM_Ar_HK_HC.html |
trend_report_FWHM_Ar_K_HC.html |
trend_report_FWHM_Ne_IZ_HC.html |
trend_report_FWHM_Ne_YJ_HC.html |
trend_report_FWHM_Ne_H_HC.html |
trend_report_FWHM_Ne_HK_HC.html |
trend_report_FWHM_Ne_K_HC.html |
trend_report_WAVEPOS_IZ_HC.html |
trend_report_WAVEPOS_YJ_HC.html |
trend_report_WAVEPOS_H_HC.html |
trend_report_WAVEPOS_HK_HC.html |
trend_report_WAVEPOS_K_HC.html |
trend_report_ARCLAMP_Ar_HC.html |
trend_report_ARCLAMP_Ne_HC.html
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QC1PAGE |
trending | associated documentation:
wave_qc1.html
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QC1PLOTS
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wave0.png
Overview plot for all detectors and up to six rotator angles showing
calibrated and rebinned arc-lamp exposures.
Missing IFUs and deviating wavelength solutions can be easily detected.
wave1.png
calibrated and rebinned arc-lamp exposures for detectors 1, 2, and 3
Note: In this example plot, IFUs 4, 11, and 15 were not operational.
wave2.png
central area of calibrated and rebinned arc-lamp exposures for detectors 1, 2, and 3
wave3.png
left column: cut in Y direction of calibrated arc-lamp images
middle column: same, central area; including reference frame if found
right column: histograms of raw frames
wave4.png
cut in Y direction of calibrated arc-lamp images with overplotted line positions
wave5.png
same, but for three enlarged areas
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QC1PARAM |
QC1 parameters written in QC1 database:
QC1 DB names: saturated_n | ar_eff_n | ne_eff_n |
ar_fwhm_mean_n | ar_fwhm_stddev_n | ne_fwhm_mean_n | ne_fwhm_stddev_n |
ar_pos_mean_n | ar_pos_maxdiff_n | ar_pos_maxdiff_id_n | ar_pos_stddev_n |
ne_pos_mean_n | ne_pos_maxdiff_n | ne_pos_maxdiff_id_n | ne_pos_stddev_n |
rot_angle_n, with n = 0, 1, ..., 6.
KMOS waves are usually taken at six different rotator angles. These fill the QC parameters
n = 1, ..., 6. The actual angles can be found in rot_angle_n.
n = 0 is reserved for the measurement at 0 degree rotator angle.
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ALGORITHM |
saturated_n: number of saturated pixels
ar_eff_n: flux in e-/s of Ar lamp
ne_eff_n: flux in e-/s of Ne lamp
ar_fwhm_mean_n: mean FWHM of Ar lines [km/s]
ar_fwhm_stddev_n: standard deviation of FWHM of Ar lines [km/s]
ne_fwhm_mean_n: mean FWHM of Ne lines [km/s]
ne_fwhm_stddev_n: standard deviation of FWHM of Ne lines [km/s]
ar_pos_mean_n: mean position offset of Ar lines [km/s]
ar_pos_maxdiff_n: maximum deviating mean position offset of Ar lines [km/s]
ar_pos_maxdiff_id_n: IFU ID with maximum deviating mean position offset
ar_pos_stddev_n: mean standard deviation of position offsets [km/s]
ne_pos_mean_n: mean position offset of Ne lines [km/s]
ne_pos_maxdiff_n: maximum deviating mean position offset of Ne lines [km/s]
ne_pos_maxdiff_id_n: IFU ID with maximum deviating mean position offset
ne_pos_stddev_n: mean standard deviation of position offsets [km/s]
rot_angle_n: rotator angle
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CERTIF |
Reasons for rejection:
low flux of arc-lamp lines
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COMMENTS |
None
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[2015-10-29T10:47:01] created by qcDocu v1.1.2, a tqs tool
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