| 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_sci.py | |||||||||||||||||||||||||||
| VERSION |
1.0 -- July 2008 1.0.1 -- changes related to scoring (June 2009) 1.0.2 -- some QC parameters replaced by pipeline values (August 2009) 1.1 -- unification with other scripts (2009-11-25) 1.1.1 -- new QC parameters: num_overexp, level_overexp (2010-03-29) 1.2 -- supporting windowed read-out (2010-04-23) 1.2.1 -- create cover sheet (2011-05-19) 1.2.2 -- skip call of scoreQC (2011-05-31) 1.2.3 -- changes needed for muc (2013-02-07) | |||||||||||||||||||||||||||
| SYNTAX | PYTHON | |||||||||||||||||||||||||||
| CALL |
processQC from $DFS_PRODUCT/ | |||||||||||||||||||||||||||
| INSTRUMENT | CRIRES | |||||||||||||||||||||||||||
| RAWTYPE | STD_NOD_OTH | STD_NOD_JIT | STD_DIR_OTH | STD_DIR_JIT | OBS_NOD_OTH | OBS_NOD_JIT | OBS_DIR_OTH | OBS_DIR_JIT | OBS_NOD_GEN | ASTRO_NOD_JIT | |||||||||||||||||||||||||||
| PURPOSE | QC check of raw standard star and science exposures, extracted spectra, and other products | |||||||||||||||||||||||||||
| PROCINPUT | raw and product standard star and science frames | |||||||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: crires_std | crires_sci | |||||||||||||||||||||||||||
| TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure: trend_report_STD_HC.html | |||||||||||||||||||||||||||
| QC1PAGE |
trending | associated documentation: std_qc1.html | |||||||||||||||||||||||||||
| QC1PLOTS top |
sci1.png 1st row: cuts through raw frames 2nd row: histograms of raw frames 3rd row: cuts through combined raw frames 4th row: overview of extracted spectra (areas that are subject to vignetting are shaded grey) sci2.png detailed view of extracted spectra sci3.png left: first raw frame middle: combined raw frames right: extraction profile frames sci4.png extracted spectra (optimal and rectangular extraction) and corresponding errors | |||||||||||||||||||||||||||
| QC1PARAM |
QC1 parameters written in QC1 database: crires_std: spec_pos | fwhm_spec | fwhm_profile | fwhm_diff | measured_iq | expected_iq | med_through | med_s2n crires_sci: spec_pos | fwhm_spec | fwhm_profile | fwhm_diff | measured_iq | expected_iq | med_s2n | |||||||||||||||||||||||||||
| ALGORITHM |
spec_pos: average position of spectrum on each detector fwhm_spec: median FWHM of the spectrum (cross-dispersion direction) fwhm_profile: median FWHM of the profile that is used in optimal extraction fwhm_diff: difference between fwhm_profile and fwhm_spec measured_iq: fwhm_spec * pixel_scale (0.086 arcsec/pixel) expected_iq: DIMM seeing corrected for airmass, telescope diameter, and wavelength med_through: median throughput (e-/photon), only if tabulated standard star flux is known med_s2n: median signal-to-noise ratio of the extracted spectra | |||||||||||||||||||||||||||
| CERTIF |
Reasons for rejection: Science products are normally not rejected; comments are written in case of unsuccessful extraction | |||||||||||||||||||||||||||
| COMMENTS | The same procedure is used for standard star and science exposures. | |||||||||||||||||||||||||||
| top | [2015-10-30T08:22:28] created by qcDocu v1.1.2, a tqs tool | |||||||||||||||||||||||||||
