| This documentation is intended both for QC scientists and SciOps astronomers (who may want to ignore the technical information displayed in grey). | |||||||||||||||||||||||
|
|||||||||||||||||||||||
| bottom plots | contact | |||||||||||||||||||||||
| NAME | sci_mos_qc_2CCD.prg | ||||||||||||||||||||||
| VERSION |
1.0 -- adapted for new pipeline (SM, 10/2006) 1.0 -- adapted for new CCDs (SM, 04/2007) | ||||||||||||||||||||||
| SYNTAX | MIDAS | ||||||||||||||||||||||
| CALL |
measureQuality from $DFS_PRODUCT/SCI_MOS/$DATE: inmidas -P -j "@@ $DFO_PROC_DIR/sci_mos_qc.prg $date $PF" | ||||||||||||||||||||||
| INSTRUMENT | FORS1 | ||||||||||||||||||||||
| RAWTYPE | SCI_MOS | ||||||||||||||||||||||
| PURPOSE | compares raw and product SCI_MOS files for FORS1 QC assessment; the plots are later reviewed within certifyProducts and stored in $DFO_PLT_DIR. | ||||||||||||||||||||||
| PROCINPUT |
raw image from AB; SCI_MOS product; | ||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: fors1_sci_mos | ||||||||||||||||||||||
| TRENDPLOT | trending | HealthCheck plot associated to this procedure: none | ||||||||||||||||||||||
| QC1PAGE | trending | associated documentation: none | ||||||||||||||||||||||
| QC1PLOTS top |
sci_mos_grap1.png extracted, sky-subtracted spectra of 4 brightest sources (black) with error spectrum (red) and extracted sky background for brightest objects (green) sci_mos_grap2.png position of a bright sky line along the slitlets sci_mos_disp1.png full display of reduced frame sci_mos_disp2.png full display of raw frame | ||||||||||||||||||||||
| QC1PARAM |
QC1 parameters written into QC1 table: QC1db names: skyline_position | skyline_rms | skyline_offset | skyline_number | avg_accuracy QC1 params created by pipeline: avg_accuracy (from wavelength calibration data) QC1 params created by this procedure: all others | ||||||||||||||||||||||
| ALGORITHM |
Description of algorithms: The whole rebinned frame is searched for emission lines. Then lines within +/- 1 pixel around skyline_position are selected and their offset with respect to the reference line is determined. The mean and rms of these offsets are stored in skyline_offset and skyline_rms. The number of skylines used is stored in skyline_number | ||||||||||||||||||||||
| CERTIF |
Reasons for rejection: - many missing slitlets or many slitlets with bad wavelength calibration - many curved slitlets - if only a few slitlets are missing or badly calibrated (offsets in sky lines, curved lines) just add a comment and certify. - skyline offsets of more than 0.3 pixels violate the nominal calibration accuracy, but may be due to temperature differences between science and calibration data and are no cause for rejection | ||||||||||||||||||||||
| COMMENTS | |||||||||||||||||||||||
| top | [2009-07-30T07:17:28] created by qcDocu v1.1, a tqs tool | ||||||||||||||||||||||
