| 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_SP_ARC.sh | |||||||||||||||||||||||
| VERSION |
1.0 -- 2006-07-25 fill template by handbook 1.1 -- 2007-12-18 upgraded for qc tutorial migration 1.2 -- 2008-04-24 writeQC replcaes call_qc1_SPARC. get_QC1 kept to fill local db | |||||||||||||||||||||||
| SYNTAX | SHELL | |||||||||||||||||||||||
| CALL |
called by processQC vio qc_SP_ARC -d $DATE -f $primfile | |||||||||||||||||||||||
| INSTRUMENT | ISAAC | |||||||||||||||||||||||
| RAWTYPE | SP_ARC | |||||||||||||||||||||||
| PURPOSE |
a) generates QC report b) writes QC1 parameters into local list The script reads the the OCS.SELECT-ARM (arm of instrument) and calls IS_SP_SA_1night.sh | |||||||||||||||||||||||
| PROCINPUT |
a) $DATE in yyyy-mm-dd, b) $primfile is the PRO.CATG=ARC_COEF product with the _0000.fits extension. c) raw frames are implicitely read from the AB. d) Reference ARC_COIEF and ARC_CORRECT are implicitely read from $DFO_QC_DIR/references. | |||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: isaac_arc | |||||||||||||||||||||||
| TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure: trend_report_OFFSETPIX_HC.html | trend_report_DISPERS_HC.html | trend_report_RESPOW_HC.html | trend_report_ARCLAMP_HC.html | trend_report_ARCXCORR_HC.html | trend_report_LW_OFFSETPIX_HC.html | trend_report_LW_DISPERS_HC.html | trend_report_LW_RESPOW_HC.html | trend_report_DISPLAM_HC.html | trend_report_RESPLAM_HC.html | trend_report_OPTDIST_SLZ_HC.html | trend_report_OPTDIST_SLJ_HC.html | trend_report_OPTDIST_SLH_HC.html | trend_report_OPTDIST_SLK_HC.html | trend_report_OPTDIST_SMZ_HC.html | trend_report_OPTDIST_SMJ_HC.html | trend_report_OPTDIST_SMH_HC.html | trend_report_OPTDIST_SMK_HC.html | trend_report_OPTDIST_LLH_HC.html | trend_report_OPTDIST_LLL_HC.html | trend_report_OPTDIST_LMJ_HC.html | trend_report_OPTDIST_LMH_HC.html | trend_report_EFFOD_SLZ_HC.html | trend_report_EFFOD_SLJ_HC.html | trend_report_EFFOD_SLH_HC.html | trend_report_EFFOD_SLK_HC.html | trend_report_EFFOD_SMZ_HC.html | trend_report_EFFOD_SMJ_HC.html | trend_report_EFFOD_SMH_HC.html | trend_report_EFFOD_SMK_HC.html | trend_report_EFFOD_LLH_HC.html | trend_report_EFFOD_LLL_HC.html | trend_report_EFFOD_LMJ_HC.html | trend_report_EFFOD_LMH_HC.html | trend_report_EFFOD_LML_HC.html | |||||||||||||||||||||||
| QC1PAGE |
trending | associated documentation: qc_IS_arc.html | |||||||||||||||||||||||
| QC1PLOTS top |
sparc0.png display MASTER_SP_FLAT for Hawaii-Double readmode on RealTimeDisplay sparc1.png Upper:Collapsed arc spectrum of the upper half array and lowe half array with two different scalings. The optical distortion corrected arc frame is used. + indicate catalog positions, converted from Angstroem to pixel using the dispersion relation. [] indicate observed arc line positions, found by the recipe after the correlation for cross-check. Central: Differences between the observed line position (converted from pixel to Angstroem using the disperison relation) and the closest catalog position. Differences are given in Angstrom. Lower: f'(x) = the 3rd order dispersion relation minus the mean linear dispersion relation. (The f`(x)=0 at x=256 (=1/4 of the array) and x=768 (=3/4 of the array) ). Differences between the observed line position (converted from pixel to Angstroem using the disperison relation) and the closest catalog position. Differences are given in Angstrom. sparc2.png Current ARC_CORRECT minus most recent ARC_CORRECT on Rtd with alternating pattern, due to usual grating offsets (~ 5pixel) sparc3.png observed arc line spectrum (Xenon or Argon lamp), and overplotted the line positions and the line flux flux scaling factor choosen such that all flux values stay within the box. | |||||||||||||||||||||||
| QC1PARAM |
QC1 parameters written into QC1 table: FITSNAME, DBNAME , typical value, description: QC.DISPCO1, qc_dispco1, dispersion coefficient QC.DISPCO2 , qc_dispco2, dispersion coefficient QC.DISPCO3 , qc_dispco3, dispersion coefficient QC.DISPCO4 , qc_dispco4, dispersion coefficient QC.WLEN , qc_wlen, central wlen QC.DISP.XCORR , qc_disp_xcorr, dispersion cross correlation QC.DISP.STDEV , qc_disp_stdev, dispersion stdev QC.ARCS.NUM , qc_arcs_num, number of found arc lines QC.ARCS.NUMGOOD , qc_arcs_numgood, number of certified arc lines QC.ARCS.NUMCAT , qc_arcs_numcat, number of arc lines in catalog QC.ARCS.NUMCATCH , qc_arcs_numcatch, number of arc lines QC.DIST1 , qc_dist1, optical distortion coeffcient QC.DISTX , qc_distx, optical distortion coeffcient QC.DISTY , qc_disty, optical distortion coeffcient QC.DISTXX , qc_distxx, optical distortion coeffcient QC.DISTYY , qc_distyy, optical distortion coeffcient QC.DISTXY , qc_distxy, optical distortion coeffcient NONE , qc_fwhm_med, median FWHM NONE , qc_pixoff, off set in pixels from nominal wavelength NONE , qc_respow, resolving power NONE , qc_arc_line_flux, arc line flux | |||||||||||||||||||||||
| ALGORITHM |
Description of algorithms: wev use the eclipse command stcube to derive mean ans stdev on certain areas | |||||||||||||||||||||||
| CERTIF |
Quality diminishing features (not under control, but tolerated) : - offsets with respect to reference wave of about 3-5 pixel - for some settings the pipeline fails Reasons for rejection: - strong slopes due to stuck filter wheels - no flux - Unsupported wavelength for the LR grating | |||||||||||||||||||||||
| COMMENTS | local difference frames (current product minus last one) and reference difference frames (current product minus reference) are provided in the detailed section of certifyProducts. Night time arcs come with one pair, day-time flats cime with one pair or one triple. | |||||||||||||||||||||||
| top | [2012-06-20T10:57:26] created by qcDocu v1.1.2, a tqs tool | |||||||||||||||||||||||
