OMEGACAM: Dome flats stability
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HC PLOTS |
dome raw u_SDSS |
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dome raw g_SDSS |
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dome raw r_SDSS |
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dome raw i_SDSS |
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dome raw z_SDSS |
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dome raw B_JOHN |
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dome raw V_JOHN |
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master dome flat level |
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number of cold pixels |
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QC1 database (advanced users):
browse |
plot
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During normal VST/OmegaCAM operations DOME flat frames are
taken for each filter for which science data was obtained, and
generally have a validity range of 4 days. They are usually
obtained during day-time calibration and consist of 5 input,
screen flat exposures (each with a flux level of about 20,000
ADU or more). The pipeline applies a bias-correction, trims the
images, and then averages them together with a 5 sigma rejection
of outliers (intended to reduce photon shot noise and to remove
cosmic rays).
The pipeline creates two output frames from its dome flat recipe
(omega_mdome): a master dome flat
(OC_MFLD_<DATE>_1_1_normal_normal_<FILTER>.fits) and a cold pixel mask
(OC_MCPM_<DATE>_1_1_normal_normal_<FILTER>.fits).
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An OmegaCAM master dome flat (single detector).
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An OmegaCAM master cold pixel map (single detector).
A value of 1 indicates a cold pixels; otherwise 0.
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DOME Flats
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
QC.RAW.DOME.MEDIAN | omegacam_dome..qc_raw_dome_median | median flux level of all input raw dome flats (ADU) | HC | | [docuSys coming] |
QC.RAW.DOME.MIN | omegacam_dome..qc_raw_dome_min | median flux level of input raw dome having the minimum average flux level (ADU) | HC | | [docuSys coming] |
QC.RAW.DOME.MAX | omegacam_dome..qc_raw_dome_max | median flux level of input raw dome having the maximum average flux level (ADU) | HC | | [docuSys coming] |
QC.MASTER.DOME.MEDIAN | omegacam_dome..qc_dome_median | median counts in normalized master dome flat (ADU) | HC | | [docuSys coming] |
QC.MASTER.DOME.STDEV | omegacam_dome..qc_dome_std | standard deviation of normalized master dome flat (ADU) | HC | | [docuSys coming] |
QC.NUMBER.COLD.PIXELS | omegacam_dome..qc_dome_cold_pixels | number of cold pixels | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The QC1 health check plots for the RAW OmegaCAM dome flats are
divided into 7 separate linked pages, each of which shows the
trending for each of 7 different filters. Since the master dome flat
produced by the OmegaCAM pipeline is normalized, it is not easy to
detect whether or not one of the input dome flat frames was either
saturated or had insufficient flux. For this reason, the raw dome
flat parameters are monitored. A further set of QC1 health check
plots exist for the OmegaCAM master dome flats monitoring both the
level and the number of detected cold pixels.
Following parameters are monitored for each of the
filters: u_SDSS, g_SDSS, r_SDSS, i_SDSS, z_SDSS, B_JOHN,
and V_JOHN:
- raw dome flats median level averaged over all 32 detectors
- raw dome flat median level for each detector
- raw dome minimum and maximum level averaged over all 32 detectors
- score outliers
Following parameters are monitored for ALL filters (possible since
the master dome flats are normalized):
- master dome flat median level averaged over all 32 detectors
- master dome flat median level for each detector
- master dome flat rms averaged over all 32 detectors
- score outliers
- number of cold pixels averaged over all 32 detectors
- number of cold pixels for each detector
- score outliers
Since the dome flat lamp is very red, the dome flats made with the
u_SDSS, the u-band quadrant of the u_g_r_i_SDSS, and even the B_JOHN
filters can have very low flux levels. This has to be tolerated as
there is no alternative dome flat lamp.
Scoring&thresholds DOME Flats
The dome flat median, as well as min/max level, averaged over all
CCDs, is scored loosely with static
thresholds. Also, the averaged number of cold pixels is scored loosely
with fixed values.
History
Date |
event |
| OmegaCAM DOME flats tend to be very stable |
2018-08-18 | CCD_75 has been failing over the last several days, replaced (PPRS-073742) |
2019-01-05 | Data taken with M1 cover closed |
2020-11-15 | CCD77 does not work; only displays random signal consistent with noise (PPRS-079377) |
2022-05-09 | CCD77 started recording some coherent signal again |
Algorithm DOME Flats
The median level and the standard deviation are calculated from the
raw input frames and master dome flats for each extension (ADU).
The qc_raw_dome_min/max correspond to the median flux level of the
input raw dome having the minimum/maximum average flux level
(ADU). These QC parameters are used to ensure that the weakest dome
flat has enough flux to create a statistically accurate master dome
flat and that the brightest does not reach the saturation limits of
the detector.
The estimate the number of cold pixels, detected in the master dome
flat frame for each extension, master domeflat is first smoothed
and divided through this smoothed image -> residual image is flat with
a level of about unity. Then a thresholding is applied which is
controlled by the following recipe parameter: --low : Low flagging
threshold for cold pixels map. [0.93] --high : High flagging threshold
for cold pixels map. [1.07] i.e. all pixels above 1.07 and below 0.93
are considered to be cold pixels.
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