| 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_SCI_IMG.sh | |||||||||||||||||||||||
| VERSION |
1.0 -- 2006-07-27 fill template by handbook 1.1 -- 2009-01-10 migrate to trendPlotter | |||||||||||||||||||||||
| SYNTAX | SHELL | |||||||||||||||||||||||
| CALL |
measureQuality from $DFS_PRODUCT/SCI_IMG/$DATE: qc_SCI_IMG -d $DATE -f $primfile | |||||||||||||||||||||||
| INSTRUMENT | ISAAC | |||||||||||||||||||||||
| RAWTYPE | SCI_IMG | |||||||||||||||||||||||
| PURPOSE |
a) calculates post-pipeline FPN and OES QC1 parameters b) generates QC report c) writes QC1 parameters into local list The script reads the DET.NCORRS.NAME (= readmode) and the OCS.SELECT-ARM (arm of instrument) and calls one IS_SIDK_1night.sh, IS_SSDK_1night.sh, IS_LGDU_1night.sh, IS_LGDD_1night.sh | |||||||||||||||||||||||
| PROCINPUT |
a) $DATE in yyyy-mm-dd, b) $primfile is the PRO.CATG=MASTER_DARK product with the _0000.fits extension. c) raw frames are implicitely read from the AB. d) Reference MASTER_DARK are implicitely read from $DFO_QC_DIR/references/DARK. | |||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: isaac_imgobs | |||||||||||||||||||||||
| TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure: trend_report_SKY_SW_HC.html | trend_report_SKY_LW_HC.html | trend_report_IQSW_HC.html | ../FULL/trend_report_IQLW_HC.html | trend_report_IQDIMM_HC.html | |||||||||||||||||||||||
| QC1PAGE |
trending | associated documentation: qc_IS_img_obs.html | |||||||||||||||||||||||
| QC1PLOTS top |
sci_img0.png display COADDED_IMG on RTD sci_img1.png UL: FWHM and flux values and error bars of all sources found by the pipeline recipe LL: FWHM, number of coadded frames Right background values within the science stack, yrange = +-10% Histogram of source FWHM Histogram of source PSF ellipticity Histogram of source PSF ellipticity orientation sci_img2.png L: jitter trace on the sky in pixel R: jitter pattern of OBJECT only frames sci_img3.png L: raw frame N minus raw frame (N-1) of the stack on the RTD, use 'SR' option in 'detailed' script. | |||||||||||||||||||||||
| QC1PARAM |
QC1 parameters written into QC1 table: FITSNAME, DBNAME , typical value, description: NONE , imgobs_min, img_obs_max, imgobs_mean ..., statistical values of science product frame NONE , no_prod, number of product frames QC.NBOBJS , objects, number of sources QC.IQ , qc_iq, image quality QC.FWHM.MODE , qc_mode, mode of the FWHM distribution QC.FWHM.ARCSEC , qc_fwhm_ac, median of the FWHM distribution QC.FWHM.PIX , qc_fwhm_pix, median of the FWHM distribution QC.NB_OBJ_F , no_obj_f, number of raw frames classified as object QC.NB_SKY_F , no_sk, number of raw frames classified as sky QC.NB_REJ_F , no_re, number of raw frames rejected for co-addition NONE , qc_absrot, mean differential absrot must be -lt 0.05 degrees NONE , qc_parang, mean differential parang must be -lt 0.05 degrees NONE , qc_ditndit, DIT * NDIT must be -lt 100 NONE , qc_skymag, instrumental magnitude of the SKY | |||||||||||||||||||||||
| ALGORITHM |
Description of algorithms: RON Median standard deviation of a serieas on N samples of 2h+1 \times 2h+1 size. The parameters h and N differ from readmode to readmode. | |||||||||||||||||||||||
| CERTIF |
Quality diminishing features (not under control, but tolerated) : - persistence in long DIT Hawaii double Darks - persistence of the throgh slit image Reasons for rejection: - DIT * NDIT > 100 - differential rotator angle larger than XXX raw frame | |||||||||||||||||||||||
| COMMENTS | NONE | |||||||||||||||||||||||
| top | [2012-06-20T10:57:39] created by qcDocu v1.1.2, a tqs tool | |||||||||||||||||||||||
