| 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 | vimos_bias.py | |||||||||||||||||||||||||||
| VERSION |
0.9 -- April 2015 1.0 -- accept both IMG_PHOT_COMBINED and IMG_OBJ_COMBINED as products (2015-10-26) | |||||||||||||||||||||||||||
| SYNTAX | PYTHON | |||||||||||||||||||||||||||
| CALL |
processQC from $DFS_PRODUCT/STD_IMG/$DATE or $DFS_PRODUCT/STD_CORO/$DATE /home/vimos/python/visir_img_std.py -i -a $AB | |||||||||||||||||||||||||||
| INSTRUMENT | VISIR | |||||||||||||||||||||||||||
| RAWTYPE | STD_IMG and STD_CORO | |||||||||||||||||||||||||||
| PURPOSE | QC checks on raw frames and products from standard stars in imaging | |||||||||||||||||||||||||||
| PROCINPUT | raw STD frames and combined product | |||||||||||||||||||||||||||
| QC1TABLE |
trending | table(s) in QC1 database: visir_zp_img | |||||||||||||||||||||||||||
| TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure: trend_report_SENS_HC.html | trend_report_SENS_Q_HC.html | trend_report_CONVER_HC.html | trend_report_CONVER_Q_HC.html | trend_report_BACKGD_N_HC.html | trend_report_BACKGD_Q_HC.html | trend_report_IQ_HC.html | trend_report_IQ_corr_HC.html | |||||||||||||||||||||||||||
| QC1PAGE |
trending | associated documentation: stdimg_qc1.html | |||||||||||||||||||||||||||
| QC1PLOTS top |
std_img1.png upper left panel: cut through combined image in X direction upper middle panel: cut through combined image in Y direction upper right panel: histrogram of combined image central left panel: cut through combined image in X direction, central area central middle panel: cut through combined image in Y direction, central area central right panel: central area of combined image std_img2.png left panel: complete combined image right panel: central area of combined image std_coro1.png same, example observation with coronographic mask std_coro2.png same, example observation with coronographic mask | |||||||||||||||||||||||||||
| QC1PARAM |
QC1 parameters written in QC1 database: QC1 DB names: sensit | conver | backgd_mean | backgd_sigma | fwhmx | fwhmy All parameters are calculated by the pipeline recipe. | |||||||||||||||||||||||||||
| ALGORITHM |
Description of algorithms: sensit: sensitivity, the estimated limiting flux expected in an 1 hour on-source integration of a point source detected with S/N of 10. Units: mJy at 10 sigma in 1 hour conver: conversion factor between ADU and Jy. F(total observed) / F(model) in ADU/Jy, where F(total observed) is the measuered and F(model) is the predicted flux backgd_mean: background level determined from the half-cycle frames backgd_sigma: noise of the background level fwhmx: FWHM (in pixels) of the fitted profile in X direction fwhmy: FWHM (in pixels) of the fitted profile in Y direction | |||||||||||||||||||||||||||
| CERTIF |
Reasons for rejection: extremely weak or invisible star | |||||||||||||||||||||||||||
| COMMENTS | NONE | |||||||||||||||||||||||||||
| top | [2015-10-29T10:49:11] created by qcDocu v1.1.2, a tqs tool | |||||||||||||||||||||||||||
