| 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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| bottom plots | contact | ||||||||||||||||||||||||||||
| NAME | kmos_skyflat.py | |||||||||||||||||||||||||||
| VERSION |
1.0 -- October 2013 1.0.1 -- usage of qc_imaovw instead of kmos_ifudsp (2014-01-28/2014-02-04) 1.0.2 -- usage of argparse module (2014-03-10) 1.0.3 -- create flux growth curves (2014-05-16) 1.0.4 -- changed cuts for ILLUM_CORR display to 0.5, 1.5 (2014-05-16) 1.0.5 -- changed cuts for ILLUM_CORR display to min-max (2014-09-11) | |||||||||||||||||||||||||||
| SYNTAX | PYTHON | |||||||||||||||||||||||||||
| CALL |
processQC from $DFS_PRODUCT/FLAT_SKY/$DATE /home/python/kmos_skyflat.py -i -a $AB | |||||||||||||||||||||||||||
| INSTRUMENT | KMOS | |||||||||||||||||||||||||||
| RAWTYPE | FLAT_SKY | |||||||||||||||||||||||||||
| PURPOSE | QC check of raw and product sky-flat exposures | |||||||||||||||||||||||||||
| PROCINPUT | raw and product sky-flat frames | |||||||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: kmos_skyflat | |||||||||||||||||||||||||||
| TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure: trend_report_SKYFLAT_NONUNIF_HC.html | trend_report_SKYFLAT_UNIF_HC.html | trend_report_SKYFLAT_MAXDEV_HC.html | |||||||||||||||||||||||||||
| QC1PAGE | trending | associated documentation: none | |||||||||||||||||||||||||||
| QC1PLOTS top |
skyflat1.png illumination correction frames for all 24 IFUs Note: IFU 13 was not operational for these example exposures skyflat2.png top: raw image of first exposure for detectors 1, 2, and 3 bottom: central area of raw images for detectors 1, 2, and 3 skyflat3.png left column: cuts in X direction through first and last raw frames right column: histograms of first and last raw frames | |||||||||||||||||||||||||||
| QC1PARAM |
QC1 parameters written in QC1 database: QC1 DB names: spat_unif | spat_maxdev | spat_maxdev_id | spat_max_nonunif | spat_max_nonunif_id | rot_angle | |||||||||||||||||||||||||||
| ALGORITHM |
spat_unif: total RMS of all illumination correction images spat_maxdev: mean illumination correction of the most deviating IFU spat_maxdev_id: IFU ID of the most deviationg IFU spat_max_nonunif: largest illumination correction RMS spat_max_nonunif_id: IFU ID of the IFU with the largest RMS rot_angle: rotator angle | |||||||||||||||||||||||||||
| CERTIF |
Reasons for rejection: the spat_max_nonunif parameter seems to be the most sensitive parameter for detecting outlying measurements | |||||||||||||||||||||||||||
| COMMENTS | KMOS sky-flats are usually measured in a sequence where the first frames is a test exposure with a low DIT. This exposure is omitted from QC processing. | |||||||||||||||||||||||||||
| top | [2015-10-29T10:47:04] created by qcDocu v1.1.2, a tqs tool | |||||||||||||||||||||||||||
