| 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 | qc_STDIMG.sh | ||||||||||||||||||||||||||||
| VERSION |
1.0 -- copied from ISAAC for NACO (2002-03-12) 1.1 -- incorporated from old NACO; new name qc_STDIMG.sh (2005-08-23) 1.2 -- 2017-08-30 docu update | ||||||||||||||||||||||||||||
| SYNTAX | SHELL | ||||||||||||||||||||||||||||
| CALL |
processQC from $DFS_PRODUCT/STDIMG/$DATE: qc_STDIMG $date $primfile " | ||||||||||||||||||||||||||||
| INSTRUMENT | NACO | ||||||||||||||||||||||||||||
| RAWTYPE | STDIMG | ||||||||||||||||||||||||||||
| PURPOSE |
The naco pipeline recipe generates a quick look image and a fits table. The fits table contains information of up to 8 sky subtracted images out of the five raw frames The QC script extracts values from the table and generates (with the help of further scripts) a nice plot | ||||||||||||||||||||||||||||
| PROCINPUT |
NACO ZPOINT_TABLE product; | ||||||||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: naco_zp | ||||||||||||||||||||||||||||
| TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure: trend_report_ZEROP_HC.html | ||||||||||||||||||||||||||||
| QC1PAGE |
trending | associated documentation: zp_qc1.html | ||||||||||||||||||||||||||||
| QC1PLOTS top |
qc_STDIMG.png upper left panel: derived zp flux in consecutives difference raw frames; upper center panel: estimated peak counts in consecutives raw frame differences; upper right panel: estimated Strehl ratio in consecutives raw frame differences; lower left panel: estimated magnitude in consecutives raw frame differences; lower center panel: estimated FWHM/arcsec on the source in consecutives raw frame differences; lower right panel: source position in the FOV in pixel; | ||||||||||||||||||||||||||||
| QC1PARAM |
QC1 parameters written into QC1 table: QC1db names: zpoint | zpoint_rms | flux_counts | fwhm_pixel/arcsec/dimm | strehl |strehl_flux/peak/rms/error FITS key names: DET.DIT | DET.NDIT | DET.NCORRS.NAME | DET.MODE.NAME | ins_filter | ins_camera | ins_dichroics | star_name/mag/mk | wfs_type | wfs_mode QC1 params created by pipeline: all QC1 params created by this procedure: none | ||||||||||||||||||||||||||||
| ALGORITHM |
Description of algorithms: For description of algorithms used by the recipe see the NACO Pipeline User Manual; | ||||||||||||||||||||||||||||
| CERTIF |
Reasons for rejection: - unusual structures or patterns (unless representative of the current state of detector); - unusual illumination, reflections, images - insufficient number of raw frames in the stack - in S13, the source migth jitter out of the FOV | ||||||||||||||||||||||||||||
| COMMENTS | Lprime and LW band zeropints use a jitter sequence not supported by the pipeline recipe. | ||||||||||||||||||||||||||||
| top | [2017-09-12T08:53:17] created by qcDocu v1.1.2, a tqs tool | ||||||||||||||||||||||||||||
