| 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 | std_mos_qc.prg | |||||||||||||||||||||||||||
| VERSION |
1.0 -- adapted for FORS2 (PS, 05/2002) | |||||||||||||||||||||||||||
| SYNTAX | MIDAS | |||||||||||||||||||||||||||
| CALL |
measureQuality from $DFS_PRODUCT/STD_MOS/$DATE: inmidas -P -j "@@ $DFO_PROC_DIR/std_mos_qc.prg $date $PF" | |||||||||||||||||||||||||||
| INSTRUMENT | FORS2 | |||||||||||||||||||||||||||
| RAWTYPE | STD_MOS | |||||||||||||||||||||||||||
| PURPOSE | compares raw and product STD_MOS files for FORS2 QC assessment; the plots are later reviewed within certifyProducts. The first plot (std_mos_grap1.png) is stored as Postscript file in $DFO_PLT_DIR. | |||||||||||||||||||||||||||
| PROCINPUT |
raw image from AB; STD_MOS product; | |||||||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: fors2_std_mos | fors2_response | |||||||||||||||||||||||||||
| TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure: trend_report_RESPONSE_300V_HC.html | trend_report_RESPONSE_300I_HC.html | trend_report_RESPONSE_600B_HC.html | trend_report_RESPONSE_600RI_HC.html | trend_report_RESPONSE_600z_HC.html | trend_report_RESPONSE_1200B_HC.html | trend_report_RESPONSE_1400V_HC.html | trend_report_RESPONSE_1200R_HC.html | trend_report_RESPONSE_1028z_HC.html | |||||||||||||||||||||||||||
| QC1PAGE | trending | associated documentation: none | |||||||||||||||||||||||||||
| QC1PLOTS top |
std_mos_grap1.png upper panel: extracted, sky-subtracted spectrum of brightest source (black) with error spectrum (green) lower panel: extracted sky background for brightest object (black) with sky lines marked (magenta) std_mos_grap2.png upper panel: efficiency (individual data in red, fit in black) lower panel: response (individual data in green, fit in black) std_mos_disp1.png full display of raw frame std_mos_disp2.png full display of reduced, sky-subtracted frame | |||||||||||||||||||||||||||
| QC1PARAM |
QC1db names: n_saturated | object_position | avg_accuracy | efficiency_ (i=1...15) QC1 params created by pipeline: avg_accuracy (from wavelength calibration data), efficiency parameters (in table) QC1 params created by this procedure: n_saturated QC1 parameters written into QC1 table: n_saturated, object_position, avg_accuracy | |||||||||||||||||||||||||||
| ALGORITHM |
Description of algorithms: n_saturated Number of pixels above 60000 counts in the raw frame within the slitlet containing the standard star spectrum. object_position Y position of standard star spectrum. | |||||||||||||||||||||||||||
| CERTIF |
Reasons for rejection: - lack of signal; - saturated spectra (flat parts in raw data; not necessarily visible in processed data) | |||||||||||||||||||||||||||
| COMMENTS | Chip 2 usually does not contain a spectrum. | |||||||||||||||||||||||||||
| top | [2015-11-05T15:16:00] created by qcDocu v1.1.2, a tqs tool | |||||||||||||||||||||||||||
