Processing IFU data from VLT instruments

Details Processing IFU data from VLT instruments Processing IFU data from VLT instruments

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006newar..50..408h&link_type=abstract

New Astronomy Reviews, Volume 50, Issue 4-5, p. 408-411.

Astronomy and Astrophysics

Astronomy

95.55.Qf, 95.75.Fg

Scientific paper

Currently three ESO/VLT instruments employ IFUs: FLAMES/GIRAFFE, VIMOS, and SINFONI. As all other VLT data, the IFU data from these three instruments are fed into a data flow system that provides, as main functions, archiving and pipeline processing. On Paranal quick-look data reduction is performed, while at Garching Headquarters quality-controlled calibration solutions and science products are produced. The pipelines also extract quality information from the data, which is fed into a database and is available for long-term performance monitoring and trending. This article focuses on the data processing and quality control processes of GIRAFFE and VIMOS data.

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