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This is the home page of the Quality Control and Data Processing
Group (QCG) within ESO's Data
Management and Operations Division (DMO). Find here information about the pipeline-processing
of data from the VLT and about their quality control.
| QuickLinks: |
| Trending
& QC1 |
Pipelines |
Data packages |
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At ESO Headquarters in Garching, data from the VLT/VLTI are
processed, their quality is checked and monitored. This is the task of the Quality
Control and Data
Processing Group ("QC Garching"). This
process forms the back-end of the Data Flow System.
QC Garching has the following main tasks:
- monitor the calibration plan and report back issues to Paranal Observatory
- create master calibration data, control their quality and
certify them
- perform instrument trend analysis and feed back the results
to Paranal Observatory
- deliver master calibration data to the science archive
- process pre-imaging data
Note:
- Since October 2011, QC Garching does not process anymore science data, due to manpower shortage.
- The creation of PI packages has also been terminated. As before, PIs can access their data on the ESO
User Portal.
General
Services:
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| www.eso.org/HC |
HealthCheck Monitor:
Information about health check parameters (daily refreshed, includes
most recent nights) |
| www.eso.org/CAL |
calChecker: calibration completeness monitor (refreshed every half hour) |
| Reference
Frames |
reference frames archive,
for daytime astronomer's use |
| QC1
Database |
download and plot QC1
parameters (advanced users) |
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Reprocessing:
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| UVES
reprocessing |
UVES ECHELLE data,
point sources: quality-controlled, homogeneous processing of complete
data set 2000-2007 |
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Find here general
information about the VLT and VLTI pipelines.
QC
related publications ...
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