The interferometric mode of the European Very Large Telescope

Details The interferometric mode of the European Very Large Telescope The interferometric mode of the European Very Large Telescope

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.160..363l&link_type=abstract

(Group of Optical and Infrared Astronomers in Japan, Astronomical Society of Japan, Inamori Foundation, et al., International Sy

Physics

Optics

Infrared Interferometers, Interferometry, Phased Arrays, Telescopes, Adaptive Optics, Near Infrared Radiation, Structural Vibration, Vibration Damping, Visible Spectrum

Scientific paper

The European Very Large Telescope (VLT) will consist of an array of four 8-m telescopes, plus two additional 2-m-class auxiliary telescopes. The two latter telescopes are fully dedicated to optical (IR and visible) interferometry, with possible combination of some or all large telescopes. This paper discusses the implementation of the VLT interferometric mode concept, which was described earlier by Lena (1987).

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