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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plots
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NAME |
flat_sky_qc_2CCD.prg
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VERSION |
1.0 -- basic functions
2.0 -- qc_report: histogram; extension to reference files
2.1 -- trend analysis
2.2 -- replaces ratio=raw1/master by diff=raw1-raw2;
fp noise determined by deriv10 now.
3.0 -- AUTO mode
3.1 -- gaussian fits to noise added
3.2 -- 4port structure evaluated
3.3 -- output to table for all 4port skyflats!
3.4 -- Low/High gain discrimination added (fpatat, 04/12/99)
Reference mode now set to fg15
3.5 -- reference column: upper frame reference; lower: closeup
of pre-/overscan regions
3.6 -- start FORS2 adaptation (fpatat 15/03/2000)
3.7 -- automatic finding of reference frame (fpatat 08/05/2000)
3.8 -- bug fixed when no filter is present (07/09/2001)
3.9 -- changed to work with the new FORS2 CCD layout (R.Mignani)
4.0 -- since noise data are not stored in QC1 DB, they are
also omitted from plot (SM, 2006-08-03)
4.1 -- changed to work with the new FORS1 CCD layout (SM, 2007-04-02)
5.0 -- adapted to new pipeline; noise calculations removed (SM, 2008-03-29)
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SYNTAX |
MIDAS
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CALL |
measureQuality
from $DFS_PRODUCT/FLAT_SKY/$DATE:
inmidas -P -j "@@ $DFO_PROC_DIR/flat_sky_qc.prg $date $PF"
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INSTRUMENT |
FORS1
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RAWTYPE |
FLAT_SKY
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PURPOSE |
compares raw and product FLAT_SKY files
for FORS1 QC assessment; the plots are later reviewed
within certifyProducts. The first plot (skyflat_grap1.png) is
stored as Postscript file in $DFO_PLT_DIR.
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PROCINPUT |
first raw flat from AB; MASTER_FLAT_SKY product;
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QC1TABLE |
trending | table(s) in QC1 database:
fors1_skyflat
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TRENDPLOT |
trending | HealthCheck plot associated to this procedure: none
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QC1PAGE |
trending | associated documentation: none
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QC1PLOTS
top |
skyflat_grap1.png
left: comparison master (red) <-> raw (black) <-> reference (green);
upper panel: middle row and middle column, full pixel range, in ADU;
lower panel: middle row and middle column, central 100 pixels, in ADU
top right: ratio master/reference
left panel: central row, full pixel range
right panel: central column, full pixel range
bottom right: histogram: all pixel values of master skyflat in log frequency histogram
skyflat_disp1.png
full display of master frame
skyflat_disp2.png
full display of 1st raw frame
skyflat_disp3.png
full display of ratio master/reference (available only for Bessell filters UBVRI, high throughput standard filters u_HIGH,b_HIGH,v_HIGH,g_HIGH and for no filter)
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QC1PARAM |
QC1 parameters written into QC1 table:
QC1db names: datancom | median_master | sigma_master
FITS key names: DATANCOM | (flat_sky_qc.prg) | (flat_sky_qc.prg)
QC1db names: median_raw | sigma_raw
FITS key names: (flat_sky_qc.prg) | (flat_sky_qc.prg)
QC1 params created by pipeline: datancom
QC1 params created by this procedure: all except datancom
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ALGORITHM |
Description of algorithms:
median_master: mean level of master skyflat within X200...1800, Y400...800 (MIDAS stat/ima; outputr(8))
sigma_master: std.dev. of master skyflat within X200...1800, Y400...800 (MIDAS stat/ima; outputr(4))
median_raw: mean level of first raw skyflat within X200...1800, Y400...800 (MIDAS stat/ima; outputr(8))
sigma_raw: std.dev. of first raw skyflat within X200...1800, Y400...800 (MIDAS stat/ima; outputr(4))
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CERTIF |
Reasons for rejection:
- remaining stars in master flat;
Smooth, large scale variations in the ratio master/reference are no reason for rejection.
Also note that the intensity of the weave-pattern variation decrases strongly from U to I.
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COMMENTS |
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[2009-07-30T07:17:04] created by qcDocu v1.1, a tqs tool
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