| 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 | QCsinfo_pupil.py | |||||||||||||||||||||||||||
| VERSION |
1.0 -- 2006-06-27 fill template by handbook 2.0 -- 2008.07.23 completely re-written in Python with added QC functions and images | |||||||||||||||||||||||||||
| SYNTAX | Python | |||||||||||||||||||||||||||
| CALL |
measureQuality from $DFS_PRODUCT/PUPIL/$DATE: QCsinfo_pupil.py -a $AB_name -i $level_of_interaction: 0-2 | |||||||||||||||||||||||||||
| INSTRUMENT | SINFONI | |||||||||||||||||||||||||||
| RAWTYPE | PUPIL | |||||||||||||||||||||||||||
| PURPOSE | a) generates QC report, b) writes QC1 parameters into local database | |||||||||||||||||||||||||||
| PROCINPUT |
No input is required: a) $DATE in now read from AB b) primary file is set in QCsinfo_pupil.py and is the PRO.CATG=MASTER_PUPIL product with the _0000.fits extension. c) raw frames are implicitly read from the AB. d) Reference MASTER_PUPIL is found and read in from $DFO_QC_DIR/references/PUPIL/. | |||||||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: sinfoni_pupil | |||||||||||||||||||||||||||
| TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure: trend_report_PUPIL_cent_HC.html | |||||||||||||||||||||||||||
| QC1PAGE |
trending | associated documentation: pupil_QC1.html | |||||||||||||||||||||||||||
| QC1PLOTS top |
pupil1.png display MED_COADD_OBJ pupil on RealTimeDisplay pupil2.png UL: Current pupil image. White dotted line denotes pupil centroid. UC: Reference pupil image. UR: (reference - current) pupil image. LL: Difference between pupil cube plane 100 and pupil cube plane 2118. LR: Filtered current pupil with guassian fit, centroid, and center values listed in legend. | |||||||||||||||||||||||||||
| QC1PARAM |
QC1 parameters, read from the RealTimeComputer of the AO module AOS.RTC.GUIDESTAR.MAGNITUDE , none AOS.RTC.OBS.FWHMMEAN , none AOS.RTC.OBS.FWHMSTD , none AOS.RTC.OBS.ENCMEAN , none AOS.RTC.OBS.ENCSTD , none AOS.RTC.OBS.STREHLMEAN , none NONE , qc_oes1, oddeven column stripe of first SKY frame, from post-pipeline QC script QC1 parameters, generated by a post-pipeline QC script that does a Gaussian fit to all planes of the final cube: X_POS , none Y_POS , none FWHM_MIN , none FWHM_MAX , none FWHM_POSANG , none FWHM_RATIO , none TOT , none QC1 parameters (a standard sequence) QC.FRMON.MEANFLUX, qc_frmon_meanflux , standard QC1 parameter: mean flux of lamp=on frame QC.FRMOFF.MEANFLUX, qc_frmoff_meanflux, standard QC1 parameter: mean flux of lamp=off frame QC.FRMDIF.MEANFLUX, qc_frmdif_meanflux standard QC1 parameter: mean flux of lamp=on frame minus lamp=off frame QC.FRMON.MAXFLUX, qc_frmon_maxflux standart QC1 parameter: max flux of lamp=on frame QC.FRMOFF.MAXFLUX, qc_frmoff_maxflux standart QC1 parameter: max flux of lamp=off frame QC.FRMDIF.MAXFLUX, qc_frmdif_maxflux standart QC1 parameter: max flux of lamp=on farme minus lam=off frame QC.FRMON.NPIXSAT , qc_frmon_npixsat Number of saturated pixels QC1 parameters for PUPIL only QC.PUPIL.X , qc_pupil_x, (20.207021), pupil center QC.PUPIL.Y , qc_pupil_y (1.741316), pupil center | |||||||||||||||||||||||||||
| ALGORITHM |
Description of algorithms: qc_pupil_x : centroid position, (weighted average) qc_pupil_y : centrid position (weighted average) | |||||||||||||||||||||||||||
| CERTIF |
Reasons for rejection: - As a technical calibration, all position values represent the instrumental/optical status. - Lamp failure might be a reason the reject the calibration. | |||||||||||||||||||||||||||
| COMMENTS | None | |||||||||||||||||||||||||||
| top | [2015-10-30T08:23:59] created by qcDocu v1.1.2, a tqs tool | |||||||||||||||||||||||||||
