| 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_STARTRACE.sh | |||||||||||||||||||||||
| VERSION |
1.0 -- 2006-07-25 fill template by handbook 1.1 -- 2008-01-09 migrate to trendPlotter plots 1.2 -- 2008-04-24 writeQC | |||||||||||||||||||||||
| SYNTAX | SHELL | |||||||||||||||||||||||
| CALL |
measureQuality from $DFS_PRODUCT/STARTRACE/$DATE: qc_STARTRACE -d $DATE -f $primfile | |||||||||||||||||||||||
| INSTRUMENT | ISAAC | |||||||||||||||||||||||
| RAWTYPE | STARTRACE | |||||||||||||||||||||||
| PURPOSE |
writes QC1 parameters into local list | |||||||||||||||||||||||
| PROCINPUT | NONE | |||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: isaac_strace | |||||||||||||||||||||||
| TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure: ../FULL/trend_report_STRACE_S_L_HC.html | ../FULL/trend_report_STRACE_I_HC.html | ../FULL/trend_report_EFFST_S_L_HC.html | |||||||||||||||||||||||
| QC1PAGE |
trending | associated documentation: qc_IS_startrace.html | |||||||||||||||||||||||
| QC1PLOTS top |
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| QC1PARAM |
QC1 parameters written into QC1 table: FITSNAME, DBNAME , typical value, description: QC.DIST1 , qc_distLR1, qc_distMR1, optical distortion coefficient QC.DISTX , qc_distLRX, qc_distMRX, optical distortion coefficient QC.DISTY , qc_distLRY, qc_distMRY, optical distortion coefficient QC.DISTXX , qc_distLRXX, qc_distMRXX, optical distortion coefficient QC.DISTYY , qc_distLRYY, qc_distMRYY, optical distortion coefficient QC.DISTXY , qc_distLRXY, qc_distMRXY, optical distortion coefficient QC.CORR_IS1 , qc_corr_IL1, qc_corr_IM1, optical distortion coefficient QC.CORR_IS2 , qc_corr_IL2, qc_corr_IM2, optical distortion coefficient QC.CORR_IS3 , qc_corr_IL3, qc_corr_IM3, optical distortion coefficient QC.FITMSE , qc_fit_mse_LR, qc_fit_mse_MR<\b> fit quality | |||||||||||||||||||||||
| ALGORITHM |
Description of algorithms: DIST optical distortion coefficients are derived from a polynomial fit to the curvature of the star traces . | |||||||||||||||||||||||
| CERTIF | The recipe requires 33 frames. Quality Control only via trending plots. | |||||||||||||||||||||||
| COMMENTS | ||||||||||||||||||||||||
| top | [2012-06-20T10:57:29] created by qcDocu v1.1.2, a tqs tool | |||||||||||||||||||||||
