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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NAME |
vimos_imgscrflt.py
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VERSION |
1.0 -- change from MIDAS to Python (February 2010)
1.0.1 -- updating qcDocu description (2011-03-07)
1.0.2 -- skip call of scoreQC (2011-05-31)
1.0.3 -- create cover sheet (2011-08-30)
1.0.4 -- changes needed for muc (2013-02-07)
1.0.5 -- changes for qc_mstplt v1.4 (2014-01-15)
1.0.6 -- changes for qc_mstdisp v1.3 (2014-01-20)
1.0.7 -- remove usage of has_key dictionary attribute (2014-03-24)
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SYNTAX |
PYTHON
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CALL |
processQC
from $DFS_PRODUCT/SFLAT_IMG/$DATE
/home/vimos/python/vimos_imgscrflt.py -i -a $AB
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INSTRUMENT |
VIMOS
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RAWTYPE |
SFLAT_IMG
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PURPOSE |
QC check on raw and product imaging lamp flats
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PROCINPUT |
products: IMG_MASTER_SCREEN_FLAT
raw frames: first raw frame
reference IMG_MASTER_SCREEN_FLAT
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QC1TABLE |
trending | table(s) in QC1 database:
vimos_scrflat
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_FLT_UB_HC.html |
trend_report_FLT_VR_HC.html |
trend_report_FLT_Iz_HC.html |
trend_report_GAIN_HC.html |
trend_report_NOISE_HC.html
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QC1PAGE |
trending | associated documentation:
scrflat_qc1.html
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QC1PLOTS
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scrflat1.png
left: first input raw frame
middle: current IMG_MASTER_SCREEN_FLAT
right: comparison to reference master flat
scrflat2.png
left: first input raw frame (central area)
middle: current IMG_MASTER_SCREEN_FLAT (central area)
right: comparison to reference master flat (central area)
scrflat3.png
cuts through current master and reference, histograms, comparison to reference
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QC1PARAM |
QC1 parameters written in QC1 database:
QC1 DB names: median_master | sigma_master | efficiency | fixp_noise | photon_noise | structure |
conad_avg | sig_conad_avg
All parameters are calculated by the pipeline recipe.
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ALGORITHM |
Description of algorithms:
median_master: median of the 1600x1800 central pixels of IMG_COMBINED_SCREEN_FLAT
sigma_master: standard deviation of the 1600x1800 central pixels of IMG_COMBINED_SCREEN_FLAT
efficiency: median of the 1600x1800 central pixels of the first input raw frame divided by
exposure time
fixp_noise: standard deviation of the 1600x1800 central pixels of the difference of the first and second
raw input flat, with the second shifted by 10x10 pixels; photon_noise is quadratically subtracted
photon_noise: standard deviation of the 1600x1800 central pixels of the difference of the first two raw
frames, divided by sqrt(2)
structure: standard deviation of the 1600x1800 central pixels of the first input raw flat with
fixp_noise and photon_noise quadratically subtracted
conad_avg: conversion factor from ADU to electrons (e/ADU). The difference frame of the first two
input raw frames is computed and the variance (square of standard deviation) of the difference frame is calculated;
the 1600x1800 central region is divided into 16x18 boxes with 100x100 pixels; for each box, the median is
calculated and divided by (2 x variance); the median value of the results from all boxes is the gain factor,
which is 1/CONAD
sig_conad_avg: standard deviation of the 16x18 CONAD values, divided by sqrt(16x18)
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CERTIF |
Imaging lamp flats are not used for data reduction; they are used for trending CONAD,
noise parameters, and filter performance.
In case of lamp failures, affected QC1 DB entries would have to be cleaned.
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COMMENTS |
none
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[2016-03-11T12:31:15] created by qcDocu v1.1.2, a tqs tool
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