Translator Disclaimer
Paper
21 July 2010 The very large telescope Interferometer: 2010 edition
Author Affiliations +
Abstract
The ESO Very Large Telescope Interferometer (VLTI) offers access to the four 8-m Unit Telescopes (UT) and the four 1.8-m Auxiliary Telescopes (AT) of the Paranal Observatory located in the Atacama Desert in northern Chile. The two VLTI instruments, MIDI and AMBER deliver regular scientific results. In parallel to the operation, the instruments developments are pursued, and new modes are studied and commissioned to offer a wider range of scientific possibilities to the community. New configurations of the ATs array are discussed with the science users of the VLTI and implemented to optimize the scientific return. The monitoring and improvement of the different systems of the VLTI is a continuous work. The PRIMA instrument, bringing astrometry capability to the VLTI and phase referencing to the instruments has been successfully installed and the commissioning is ongoing. The possibility for visiting instruments has been opened to the VLTI facility.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
PROCEEDINGS
11 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

The Very Large Telescope Interferometer: an update
Proceedings of SPIE (July 28 2008)
The Very Large Telescope Interferometer v2012+
Proceedings of SPIE (September 12 2012)
Interferometry with the ESO Very Large Telescope
Proceedings of SPIE (August 23 1995)
The VLTI: a status report
Proceedings of SPIE (February 21 2003)

Back to Top