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| QC PLOTS |
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CURRENT |
HISTORY |
| Daily Health Checks: |
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| flux range |
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| QC1 hawki_dark database (advanced users):
browse
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plot
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Click on CURRENT to see the last trending (Health Check).
Click on HISTORY to see the historical evolution of the trending. |
This tutorial provides information for the the
TW Flats
Health Check trending.
The TW Flats trending is based on the measurement
of QC1 parameters from the twilight flat field calibration
data. Following the calibration plan, the twilight flat fields are taken during evening (usually)
and morning (rarely) twilights with clear skies as
required for the calibration of SCIENCE data.
HAWK-I instrument does not have an internal lamp. In the infrared, twilight flats
are taken in a manner to sample a large flux range by integrating on the
twilight sky as the sun sets or rises. Twilight flats are therefore,
one of the most time critical calibrations, since of the narrow time
window. This is also the reason why more operational related quality
parameters like the covered flux range are monitored for twilight flat
calibrations.
The standard deviations of the pixel values of each detector in the
MASTER FLAT image are monitored in J, H, Ks & Y filters.
QC1 parameters
- flux range within raw frame stack (QC1 database table hawki_twflat, column qc_flat_medstdev, product keyword QC.FLAT.MEDSTDEV)
Description: The standard deviation of the raw frame fluxes as a rough measure of the covered flux range.
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