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 |
dark_blue.prg
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VERSION |
1.4
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SYNTAX |
MIDAS
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CALL |
from $DFS_PRODUCT/BIAS_BLUE/$DATE:
uves.MeasureQuality -a <AB> -c dark_blue.prg [-i|--NOingestQC1pars]
where
<AB> is the Association Block
[-i] forces QC1 parameter ingestion (default)
[--NOingestQC1pars] prevents QC1 parameter ingestion
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INSTRUMENT |
UVES
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RAWTYPE |
DARK_BLUE & PDARK_BLUE
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PURPOSE |
Comparison of raw, master and reference DARK and PARSITIC-DARK files
for UVES QC assessment;
QC1 values are calculated and fed into the QC1 table.
QC1 plot(s) and/or display(s) are generated,
and later reviewed within certifyProducts.
The generated plots stored in $DFO_PLT_DIR/$DATE
with the name r.<DPid>_tpl_0000.fits.png where <DPid>
is the Data Product Identification of the first frame of the
template.
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PROCINPUT |
first raw DARK frame from AB; MASTER_DARK_BLUE or MASTER_PDARK_BLUE, and MASTER_BIAS_BLUE from AB
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QC1TABLE |
trending | table(s) in QC1 database:
uves_dark
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
HEALTH/trend_report_DARK_SM_HC.html
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QC1PAGE |
trending | associated documentation:
detmon_qc1.html
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QC1PLOTS
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dark_blue.montage.png
A montage image made up of the following individual reports simply for the purposes
of easier/better display in XV during the certification process. Created together
with the reference montage (see below) within the uves.MeasureQuality script.
Can be recreated manually by calling the script
uves.makeQCreportMontage -a <AB>, see uves.makeQCreportMontage -h for more details.
dark_blue.montage.ref.png
A montage image made up from the individual QC reports of the reference AB located by
the script uves.getRefAB. During certification, the two montage images are blinked to
facilitate identification of unusual features. This reference montage created at the
same time as the AB montage (see above).The montage of the reference AB is easily
identified during the blinking as the one with the grey background.
dark_blue_0000.fits.png
box1: comparison of master DARK (red) <-> raw DARK (black) <-> master BIAS (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
box 2: histogram: all pixel values in log frequency histogram; raw DARK: black, master BIAS: green; there should be a dominant
peak with Gaussian shape (which translates to parabola shape in this log freq diagram)
box 3: histogram: log frequency histogram; master DARK: red; upper panel: all pixel values, there should be a dominant
peak with Gaussian shape (which translates to parabola shape in this log freq diagram); lower panel: closeup
arount zero where the mean DARK current is expected to be close to
top panel: name of analyzed master DARK frame and name of the master BIAS frame used for comparison (and by the pipeline)
bottom panel: some template properties and QC1 parameters
dark_blue_0000.fits_1.ima.png
full display of raw frame
dark_blue_0000.fits_2.ima.png
full display of master frame (box: area to be displayed in bias_blue_0000.fits_3.png)
dark_blue_0000.fits_3.ima.png
closeup display of master frame
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QC1PARAM |
QC1 parameters written into QC1 table:
QC1db names: mean_raw | mean_dark | current_dark | exptime
FITS key names: <qc_script> | <qc_script> | <qc_script> | EXPTIME
QC1 params created by pipeline: None
QC1 params created by this procedure: mean_raw | mean_dark | current_dark
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ALGORITHM |
Description of algorithms: Algorithms for pipeline created keywords are (in principal) described in the pipeline user's manual
- mean_raw: mean value of raw frame, this QC parameter is currently calculated by the QC report script, not by the pipeline.
Description: computed with the MIDAS command:
stat/ima <FIRST_RAW_FRAME> [@{CENTX1},@{CENTYR1}:@{CENTX2},@{CENTYR2}] option=S
CENTX1, CENTYR1, CENTX2 & CENTYR2 define a central 100x100 pixel region
- mean_dark: mean value across master dark, this QC parameter is currently calculated by the QC report script, not by the pipeline.
Description: computed with the MIDAS command:
stat/ima <PRO.CATG=MASTER_[P]DARK_BLUE> [@1,@1:@{XEND},@{YEND}] bins=1 exc={lower_master},{upper_master}
XEND & YEND are the full sizes of the chips.
lower_master & upper_master are half of and twice the means of the central regions of the MASTER DARK frame.
- current_dark: mean_dark normalized to 3600 secs exposure time, this QC parameter is currently calculated by the QC report script, not by the pipeline.
Description: computed with the MIDAS command:
current_dark = mean_dark/EXPTIME*3600
- exptime: exposure time in secs., this QC parameter is taken directly from the header of the first RAW file, it propagates to the PRODUCT file(s) unchanged by the pipeline, product keyword EXPTIME.
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CERTIF |
Reasons for rejection:
For DARKs:
- less than three frames in a DARK frame set
- differing exposure times in the frame set (often because the last frame is stopped early)
- very short exposure times (less than 1000sec, normal exposure time is 3600 sec, anything less than this is probably a TEST frame or similar)
PDARKs are never rejected as these are technical calibrations.
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COMMENTS |
See also the PDARK trending plot here.
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[2015-10-30T08:20:33] created by qcDocu v1.1.2, a tqs tool
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