Translator Disclaimer
Paper
16 September 2004 VLT interferometry in the data flow system
Author Affiliations +
Abstract
Science interferometry instruments are now available at the Very Large Telescope for observations in service mode; the MID-Infrared interferometry instrument, MIDI, started commissioning and has been opened to observations in 2003 and the AMBER 3-beam instrument shall follow in 2004. The Data Flow System is the VLT end-to-end software system for handling astronomical observations from the initial observation proposal phase through to the acquisition, archiving, processing, and control of the astronomical data. In this paper we present the interferometry specific components of the Data Flow System and the software tools which are used for the VLTI.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Pascal Ballester, Tom Licha, Derek J. McKay, Isabelle Percheron, Michele Peron, Andrea Richichi, Cyrus Sabet, and Markus Wittkowski "VLT interferometry in the data flow system", Proc. SPIE 5493, Optimizing Scientific Return for Astronomy through Information Technologies, (16 September 2004); https://doi.org/10.1117/12.551098
PROCEEDINGS
8 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

Data flow system for the very large telescope interferometer
Proceedings of SPIE (November 01 2001)
Imaging from the first 6-beam infrared combiner
Proceedings of SPIE (September 12 2012)
Recent progress at the CHARA interferometric array
Proceedings of SPIE (June 27 2006)
Imaging rapid rotators with the PAVO beam combiner at CHARA
Proceedings of SPIE (September 12 2012)
MIDI scientific and technical observing modes
Proceedings of SPIE (February 21 2003)
Scientific observations with MIDI on the VLTI present and...
Proceedings of SPIE (October 20 2004)
Recent progress on the infrared Michelson array
Proceedings of SPIE (August 01 1990)

Back to Top