| 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 | crires_dark.py | |||||||||||||||||||||||||||
| VERSION |
1.0 -- July 2008 1.0.1 -- logging, option parsing, and module import changed (2009-03-19) 1.0.2 -- supporting numpy V1.3 and matplotlib V0.99 (2009-10-29) 1.1 -- support for windowed read-out mode (2010-04-27) 1.1.1 -- create cover sheet (2011-05-19) 1.1.2 -- skip call of scoreQC (2011-05-31) 1.1.3 -- changes needed for migration to muc (2013-02-06) | |||||||||||||||||||||||||||
| SYNTAX | PYTHON | |||||||||||||||||||||||||||
| CALL |
processQC from $DFS_PRODUCT/DARK/$DATE /home/python/crires_dark.py -i -a $AB | |||||||||||||||||||||||||||
| INSTRUMENT | CRIRES | |||||||||||||||||||||||||||
| RAWTYPE | DARK | |||||||||||||||||||||||||||
| PURPOSE | QC check of raw and product dark exposures | |||||||||||||||||||||||||||
| PROCINPUT | raw, product, and reference dark frames | |||||||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: crires_dark | |||||||||||||||||||||||||||
| TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure: trend_report_DARKMED_HC.html | trend_report_DARKRON_HC.html | |||||||||||||||||||||||||||
| QC1PAGE |
trending | associated documentation: dark_qc1.html | |||||||||||||||||||||||||||
| QC1PLOTS top |
dark1.png left: current master dark, one plot per detector right: current dark - reference dark, one plot per detector dark2.png as first image, central regions per detector dark3.png cuts through raw and master, histrograms, comparison to reference | |||||||||||||||||||||||||||
| QC1PARAM |
QC1 parameters written in QC1 database: QC1 DB names: darkmed | ron12 | ron23 | dark_stddev | |||||||||||||||||||||||||||
| ALGORITHM |
darkmed: average of the median values of the input frames ron12: subtract first input frame from second; compute standard deviation for 100 sub images of 13x13 pixels; read-out noise is median of these values multiplied with sqrt(NDIT/2) ron23: same as ron12 but with second frame subtracted from third dark_stddev: standard deviation of the median values of the input frames | |||||||||||||||||||||||||||
| CERTIF |
Reasons for rejection: unusual high dark level or read-out noise, unusual structure | |||||||||||||||||||||||||||
| COMMENTS |
There should be reference frames for all standard DIT values (see User Manual): 1, 2, 3, 5, 7, 10, 15, 20, 30, 45, 60, 90, 120, 180, 300, and 600 secs. | |||||||||||||||||||||||||||
| top | [2015-10-30T08:22:19] created by qcDocu v1.1.2, a tqs tool | |||||||||||||||||||||||||||
