OMEGACAM: System efficiency
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HC PLOTS |
zeropoint u_SDSS |
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zeropoint g_SDSS |
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zeropoint r_SDSS |
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zeropoint i_SDSS |
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zeropoint z_SDSS |
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zeropoint B_JOHN |
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zeropoint V_JOHN |
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fwhm u_SDSS |
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fwhm g_SDSS |
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fwhm r_SDSS |
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fwhm i_SDSS |
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fwhm z_SDSS |
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fwhm B_JOHN |
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fwhm V_JOHN |
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ellipticity u_SDSS |
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ellipticity g_SDSS |
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ellipticity r_SDSS |
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ellipticity i_SDSS |
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ellipticity z_SDSS |
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ellipticity B_JOHN |
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ellipticity V_JOHN |
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QC1 database (advanced users):
browse |
plot
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During normal VST/OmegaCAM operations standard star frames
(DPR.TYPE = STD,ZEROPOINT) are taken on the same night matching
each filter for which science data was obtained. The data
consists of a single standard star field of similar airmass and
identical filter. To monitor the ambient conditions (extinction)
another standard star observation is made of the polar field
(DPR.TYPE = STD,EXTINCTION) at the beginning, middle, and end of
the night.
The standard frame is bias corrected, flat-fielded, background
subtracted, and trimmed. SExtractor is run on the image and is
cross-matched to sources present in the external standard star
catalogue (REFERENCE_STAR_CATALOG). The apparent magnitudes of the
SExtractor catalogue and the absolute magnitudes of the
REFERENCE_STAR_CATALOG is used to define the zeropoints for each
detector. The zeropoints monitored for the health check plots are
derived from flux units of electrons/second.
The pipeline creates four output frames from its standard star recipe
(omega_standard_star): a reduced standard star image
(OC_PSTD_<DATE>_1_1_normal_normal_<FILTER>.fits), a photometric fits
table listing each secondary standard star source detected in each
detector (OC_PPHO_<DATE>_1_1_normal_normal_<FILTER>.fits), a fits
table listing the computed zeropoints for each detector
(OC_PZPT_<DATE>_1_1_normal_normal_<FILTER>.fits), and a mask of bad
pixels, saturated pixels, and satellite trails for the reduced
standard star image (OC_PSMA_<DATE>_1_1_normal_normal_<FILTER>.fits).
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The full OmegaCAM reduced standard frame (r_SDSS filter).
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A single detector (ESO_CCD_#71) OmegaCAM reduced standard frame (r_SDSS filter).
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A single detector (ESO_CCD_#71) OmegaCAM reduced standard mask (r_SDSS filter).
A value of 1 indicates a bad pixel; otherwise 0.
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Standard Star Zeropoint
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
QC.ZEROPOINT_ELECTRON | omegacam_std..qc_zeropoint_electron | detector zeropoint computed from flux units of e-/sec. | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
Following parameters are monitored for each of the
filters: u_SDSS, g_SDSS, r_SDSS, i_SDSS, z_SDSS, B_JOHN,
and V_JOHN:
- zeropoint as averaged over all 32 detectors
- zeropoint rms averaged over all 32 detectors
- zeropoints for each individual detector
- score outliers
Scoring&thresholds Standard Star Zeropoint
Very loose scoring applied.
History
Date |
event |
2012-12-05 | System throughput increased by 5% due to washing of M1 |
2013-12-05 | System throughput drop by about 0.6% within a few days early December, due to dust. Stable since then. |
2014-03-27 | The M1 was washed. This resulted in an improvement of ~3.8% in the mirror's reflectivity. |
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 Standard Star Zeropoint
The detector-specific zeropoint computed from flux units of electrons/second.
Standard Star Image Quality
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
[calculated by QC procedure] | omegacam_std..qc_delta_fwhm | difference (qc_std_seeing - qc_ambi_seeing) (arcsec) (QCscript) | HC | | [docuSys coming] |
QC.STD.SEEING | omegacam_std..qc_std_seeing | median Sextractor FWHM of detected sources with STAR_CLASS>=0.9 (arcsec) | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
Following parameters are monitored for each of the
filters: u_SDSS, g_SDSS, r_SDSS, i_SDSS, z_SDSS, B_JOHN,
and V_JOHN:
- image quality plotting the stellar source FWHM vs. the corrected (for airmass and waveband) DIMM seeing (arcsec)
- the difference in the standard star FWHM vs. the corrected DIMM seeing (arcsec)
- score outliers
A one-to-one comparison of the image quality (the FWHM of the stars
matched from the secondary standard catalogue) achieved by OmegaCAM
and the seeing as measured by the DIMM (converted to the STD star OB's
airmass and waveband) are plotted against one another (in arcsec). The
values for each of the 32 detectors is shown.
Scoring&thresholds Standard Star Image Quality
Not scored.
History
No major events.
Algorithm Standard Star Image Quality
The FWHM (arcsec) is measured only for sources identified as stellar (CLASS_STAR >= 0.90 from the SExtractor detection)
and are contained in the pipeline product frame PRO.CATG=ZEROPOINTS.
The DIMM seeing has been adjusted to the wavelength and airmass of the
standard star observation.
Standard Star Ellipticity
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
QC.STD.ELLIPTICITY | omegacam_std..qc_std_ellipticity | median Sextractor ellipticity of detected sources with STAR_CLASS>=0.9 | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
Following parameters are monitored for each of the
filters: u_SDSS, g_SDSS, r_SDSS, i_SDSS, z_SDSS, B_JOHN,
and V_JOHN:
- the stellar source ellipticity (1 - b/a) averaged over all 32 detectors
- the stellar source ellipticity rms averaged over all 32 detectors
- the stellar source ellipticity for each individual detector
- score outliers
Scoring&thresholds Standard Star Ellipticity
Very loose scoring applied.
History
No major events.
Algorithm Standard Star Ellipticity
The ellipticity (1 - b/a) is measured only for source identified as
stellar (CLASS_STAR >= 0.90 from the SExtractor detection) and is
contained in the pipeline product frame PRO.CATG=ZEROPOINTS
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