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 |
std_lss_qc.prg
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VERSION |
1.0 -- adapted for FORS2 (PS, 05/2002)
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SYNTAX |
MIDAS
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CALL |
measureQuality
from $DFS_PRODUCT/STD_LSS/$DATE:
inmidas -P -j "@@ $DFO_PROC_DIR/std_lss_qc.prg $date $PF"
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INSTRUMENT |
FORS2
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RAWTYPE |
STD_LSS
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PURPOSE |
compares raw and product STD_LSS files
for FORS2 QC assessment; the plots are later reviewed
within certifyProducts. The first plot (std_lss_grap1.png) is
stored as Postscript file in $DFO_PLT_DIR.
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PROCINPUT |
raw image from AB; STD_LSS product;
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QC1TABLE |
trending | table in QC1 database: none
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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
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std_lss_grap1.png
left:
upper panel: extracted, sky-subtracted spectrum of brightest source (black) with error spectrum (green)
lower panel: extracted sky background for brightest object (black) with sky lines marked (magenta)
std_lss_disp1.png
full display of raw frame
std_lss_disp2.png
full display of reduced, sky-subtracted frame
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QC1PARAM |
QC1 parameters written into QC1 table: none
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ALGORITHM |
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CERTIF |
Reasons for rejection: - lack of signal; - saturated spectra (flat parts)
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COMMENTS |
Chip 2 usually does not contain a spectrum.
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[2015-11-05T15:15:58] created by qcDocu v1.1.2, a tqs tool
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