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 |
xshooter_dark.py
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VERSION |
: 1.0 -- July 2008
: 1.1 -- May 2009, adapted for from xshooter_bias.py
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SYNTAX |
PYTHON
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CALL |
processQC
from $DFS_PRODUCT/DARK_UVB/$DATE:
from $DFS_PRODUCT/DARK_VIS/$DATE:
$DFO_PROC_DIR/python/xshooter_dark.py -i -a $AB
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INSTRUMENT |
XSHOOTER
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RAWTYPE |
DARK_AGC
DARK_UVB
DARK_VIS
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PURPOSE |
compares raw and product DARK_UVB/VIS files
for XSHOOTER QC assessment; the plots are later reviewed
within certifyProducts. The plot is stored in $DFO_PLT_DIR.
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PROCINPUT |
first pre-processed DARK; MASTER_DARK product;
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QC1TABLE |
trending | table(s) in QC1 database:
xshooter_dark
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_DET_AGC_dark_HC.html |
trend_report_DET_UVB_dark_HC.html |
trend_report_DET_VIS_dark_HC.html
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QC1PAGE |
trending | associated documentation:
dark_qc1.html
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QC1PLOTS
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dark_UVB_X00.png
top left: comparison of central row in first (black) and last (green) raw file
top center: comparison of central column in first (black) and last (green) raw file
top right: histogram of flux in master (red)
bottom left: comparison of central part of central row in first (black) and last (green) raw file
bottom center: comparison of central part of central column in first (black) and last (green) raw file
bottom right: average flux in rows (dark blue) and columns (light blue) of master frame
dark_UVB_A00.png
full display of UVB first raw and master frame
dark_VIS_X00.png
top left: comparison of central row in first (black) and last (green) raw file
top center: comparison of central column in first (black) and last (green) raw file
top right: histogram of flux in master (red)
bottom left: comparison of central part of central row in first (black) and last (green) raw file
bottom center: comparison of central part of central column in first (black) and last (green) raw file
bottom right: average flux in rows (dark blue) and columns (light blue) of master frame
dark_VIS_A00.png
full display of VIS first raw and master frame
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QC1PARAM |
QC1 parameters written into QC1 table:
QC1db names: median_dark | mean_dark | sigma_dark | cosmic_rate | avg_cosmic
FITS key names: QC.MDARKMED | QC.MDARKAVG | QC.MDARKRMS | QC.CRRATE | QC.NCRH.AVG
QC1db names: fixed_pattern | error_fixed_pattern | fp_norm | error_fp_norm
FITS key names: QC.FPN | QC.FPN.ERR | QC.NORMFPN | QC.NORMFPN.ERR
QC1 params created by pipeline: all
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ALGORITHM |
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CERTIF |
Reasons for rejection: - remnants from redmost echelle orders (right side)
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COMMENTS |
There is no QC report for dark frames acquired with the acquisition and guiding camera (AGC) CCD
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[2020-10-08T05:44:25] created by qcDocu v1.1.2, a tqs tool
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