CRIRES: Dark
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HC PLOTS |
Dark median |
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Dark median YJHK bands |
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Dark median LM bands |
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Read-Out Noise |
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Dark nbad |
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QC1 database (advanced users):
browse |
plot
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Dark frames are taken daily as part of the calibration plan in sets
of 3 frames for each DET.SEQ1.DIT value. Darks in specific setups:
INS.WLEN.ID=Y1029, J1232, H1559, K2217, L3377, M4266, with short and
long DIT are taken every day as health checks. Darks in other setups
are only measured when they are triggered by settings of science data
observed during the night.
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Example of the DET.WLEN.ID=J1232, DET.SEQ1.DIT=10.0 sec
dark frames for all 3 detectors.
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Information about the Quality Control performed utilizing dark
frames of the instrument BEFORE the upgrade (before 2021-09)
can be found here.
DARK level
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
QC.DARK.MEDIAN | criresp_dark..dark_median | median dark level of input frames | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The
median dark level is trended for each detector, as
well as for YJHK and LM bands, separately.
Scoring&thresholds DARK level
The dark_median of the J1228 wavelength setup
master darks is tightly scored, with dynamic
thresholds following the median average of the current
period. The only requirement on the dark current is stability on the calibration timescale.
History
Date |
event |
2021-10-01 | beginning of operations of the upgraded CRIRES |
Algorithm DARK level
Group the input frames by different values of DET.SEQ1.DIT and
WLEN.ID; Load the images and create the associate error for
each of them; Collapse the images; Compute BPM from the
collapsed master dark; The median level of master dark is
calculated for each detector.
DARK RON
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
QC.DARK.RON1 | criresp_dark..dark_ron1 | RON whole frame raw2-raw1 | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The
read-out noise (RON) is trended for each detector,
selected setups.
Scoring&thresholds DARK RON
The ron1 is scored, with dynamic
thresholds following the median average of the current
period. The only requirement on the dark RON is stability on the calibration timescale.
History
Date |
event |
2021-10-01 | beginning of operations of the upgraded CRIRES |
Algorithm DARK RON
Group the input frames by different values of DET.SEQ1.DIT and
WLEN.ID; Load the images and create the associate error for
each of them; Collapse the images; Compute BPM from the
collapsed master dark; The RON is derived from difference
between 2nd and 1st input frame, ron1, and between 3rd and
2nd, ron2) of the master dark; It is
calculated for each detector.
DARK NBAD
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
QC.DARK.NBAD | criresp_dark..dark_nbad | number of bad pixels in master dark | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The
number of bad pixels (nbad) is trended for each detector,
selected setup.
Scoring&thresholds DARK NBAD
The dark_nbad is scored, with dynamic
thresholds following the median average of the current
period. The only requirement on the dark number of bad
pixels is stability on the calibration timescale.
History
Date |
event |
2021-10-01 | beginning of operations of the upgraded CRIRES |
Algorithm DARK NBAD
Group the input frames by different values of DET.SEQ1.DIT and
WLEN.ID; Load the images and create the associate error for
each of them; Collapse the images; Compute BPM from the
collapsed master dark; The number of bad pixels is calculated
where the bad pixels are those that deviate from average
signal; It is calculated for each detector.
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