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This is the home page of the Quality Control and Data Processing
Group (QCG) which is part of the Data Products Department (DPD) at the 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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Our mission statement ...
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:
Calibration data
- 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
Science data
- reduce science data (taken in Service Mode or Visitor Mode)
and control their quality
- organize and distribute all data (taken in Service Mode or
Visitor Mode) (all VLT and VLTI instruments)
- process pre-imaging data
Note:
- Since July 2009, all science
data are processed by QC Garching, no matter if taken in Service Mode or
Visitor Mode. Before that date, only
Service Mode runs were supported.
- Since P83 (April 2009), all PIs can
access their data packages on the ESO
User Portal.
General
Services:
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| www.eso.org/HEALTH |
HealthCheck Monitor:
Information about health check parameters (daily refreshed, includes
most recent nights) |
| 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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