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Quality Control provides the tools necessary for the calibration of
the VLT instruments and the assessment of the data quality. For this
purpose the system includes:
- the Calibration Plan maintained by the Instrument Scientist
and describing the rules and recipes, calibration and physical data,
as well as instrument descriptions, necessary for a given instrument.
- the Calibration Server, a local database structure storing all the
above products. Applications allow to verify the data stored in the
calibration server and submit them to the central archive.
- Instrument Models, ranging from ETCs to imaging simulations allowing
to predict and control instrument performance.
The main activity of Quality Control is to monitor the performance
of the pipeline and to assess the data quality. To this end the
following systems are regularly monitored:
- Pipeline
- Detector and calibration units
- Observation conditions (e.g. sky background)
- Instrument function testing: focus, instrument response
- Instrument
- Specific testing: scattered light, non-linearities
- Comparisons to instrument models
- Certification of the master calibration data
- Observatory
- Cross-correlations
- Trend analysis
Number of the above tasks
will be implemented in the Quality Control pipeline and be executed during
observations. Another part will be available in the form of
interactive procedures for use by the DFIR. If a problem is identified
which relates to the instrument, the DFIR will make use of a central
problem report system.
An aspect of the Quality Control will be the production and
maintenance of instrument models for the purpose of exposure time
calculation and control of the instrument efficiency.
ESO local web document owner
Thu Feb 20 18:11:39 MET 1997