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 |
QCocam_bias.py
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VERSION |
1.0 -- 2012-06-10 First draft of this QC report
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SYNTAX |
Python
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CALL |
measureQuality of data contained in $DFS_PRODUCT/BIAS/$DATE
within processQC: processQC -a $AB
explicit call: QCocam_bias.py -a [$AB_name] -e [$ext_number: 1-32] -i [$level_of_interaction: 0-2]
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INSTRUMENT |
OMEGACAM
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RAWTYPE |
BIAS (DPR.TYPE = BIAS)
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PURPOSE |
a) generates 2 QC reports for each OmegaCAM CCD
b) writes QC1 parameters into local QC1 database omegacam_bias
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PROCINPUT |
No input is required:
a) $DATE is read from AB
b) the primary file is set in QCocam_bias.py and is the PRO.CATG=MASTER_BIAS product with the _0000.fits extension.
c) raw frames are implicitly read from the AB.
d) All reference products: MASTER_BIAS and HOT_PIXELS_MAP, are found and read in from $DFO_ROOT_DIR_FC/calib/references/BIAS/.
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QC1TABLE |
trending | table(s) in QC1 database:
omegacam_bias
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TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_BIAS_level_HC.html
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QC1PAGE |
trending | associated documentation:
bias_QC1.html
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QC1PLOTS
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bias1.png
display each of 32 MASTER_BIAS frames on ds9 display.
bias2.png
display each of 32 HOT_PIXELS_MAP frames on ds9 display. Note that hot pixels have a value of 1. Normal pixels = 0.
bias3.png
left: full-field image of the master bias of the extension listed at the top of the image
center left: 4x zoom of the center area of the master bias
center right: the difference of the reference master bias and the current master bias frames.
The median level of the difference image is listed to the right of the frame.
right: full-field image of the hot pixels map. The positions of the reference frame hot pixels are shown
in red, while the hot pixels of the current bias frame are shown in blue. The total numbers of hot pixels are listed
in the frame legend.
bias4.png
top left: a) three single column traces of the current/reference master bias through:
x = 256 (dark grey)
x = 1024 (middle grey)
x = 1792 (light grey)
b) average of all columns (normalized) of current master bias (thick blue line)
c) average of all columns (normalized) of reference master bias (thick red line)
top center: a) three single row traces of the current/reference master bias through:
y = 256 (dark grey)
y = 2048 (middle grey)
y = 3840 (light grey)
b) average of all rows (normalized) of current master bias (thick blue line)
c) average of all rows (normalized) of reference master bias (thick red line)
top right: a) logarithmic histogram of current master bias (blue line)
b) logarithmic histogram of reference master bias (red line)
The median levels (as computed from a Gaussian fit) are shown as vertical dashed lines and listed in the legend.
lower left: difference between the average column traces of the reference and current master bias frames
lower center: difference between the average row traces of the reference and current master bias frames
In both plots, the zero line is shown in orange as a reference.
lower right: logarithmic histogram of the difference between the reference and current master bias frames.
Ideally, the histogram should straddle the zero line (shown in orange).
The median difference (as computed from a Gaussian fit) is shown as vertical dashed green line.
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QC1PARAM |
QC1 parameters written into QC1 table(omegacam_bias)
SOURCE(header or script) DBNAME value description
PRO.DATANCOM datancom 10 number of raw files combined in pipeline processing
QC.MASTER.BIAS.MEDIAN qc_bias_median 276.455 median value of master bias frame (ADU)
QC.MASTER.BIAS.STDEV qc_bias_std 0.8692 standard deviation of master bias frame (ADU)
QC.NUMBER.HOT.PIXELS qc_bias_hotpixels 98 number of hot pixels in master bias frame
QCocam_bias.py qc_temp_mosaic_plate 146.5 average temperature probe of mosaic plates from DET.TLM5/8 (QC script)
QCocam_bias.py qc_fpn -0.0043421 fixed pattern noise in master bias (ADU) (QC script)
QCocam_bias.py qc_delta_bias_median 1.45 median difference of reference - current master bias (ADU) (QC script)
QCocam_bias.py qc_delta_bias_hotpixels 15 difference in no. of hot pixels: reference - current master bias (QC script)
QCocam_bias.py qc_delta_bias_fpn 0.0012581 difference in fpn: reference - current master bias (ADU) (QC script)
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ALGORITHM |
Description of algorithms:
qc_bias_median: the master bias frame is created from 10 input, zero-second bias exposures, averaged together with a 5sigma rejection
of outliers (where sigma is defined from the dispersion of each pixel through the 10 input frames). This QC parameter is the median level of
this master bias frame.
qc_bias_std: the standard deviation of the master bias frame.
qc_bias_hotpixels the number of hot pixels in the master bias frame.
qc_fpn: a central region [{100, 100)-->(1948, 4000)] of the master bias frame is defined, shifted by 10 pixels in both x and y, and
subtracted from itself. The statistics of the difference image determines the fixed pattern noise.
qc_delta_bias_median: median difference of reference - current master bias (ADU).
qc_delta_bias_hotpixels: the difference in the number of hot pixels between the reference and current master bias frames.
qc_delta_bias_fpn: the difference in fixed-pattern-noise between the reference and current master bias frames.
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CERTIF |
- The master bias frames from detectors ESO_CCD_#68 and #90 have a pronounced central ridge. This is stable and can be well subtracted.
Therefore, these features are tolerated, but can create a larger number of hot pixels when compared to other detectors.
- A sudden change in the bias level of any detector, or the presence of pronounced structure should be reported to Paranal and the
master bias rejected.
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COMMENTS |
OmegaCAM bias frames are normally taken daily and consist of 10 raw, zero-second exposures.
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[2015-11-05T15:13:29] created by qcDocu v1.1.2, a tqs tool
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