Magdalena Ridge Observatory optical interferometer: a status report

Details Magdalena Ridge Observatory optical interferometer: a status report Magdalena Ridge Observatory optical interferometer: a status report

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.4838..113l&link_type=abstract

Interferometry for Optical Astronomy II. Edited by Wesley A. Traub. Proceedings of the SPIE, Volume 4838, pp. 113-118 (2003).

Astronomy and Astrophysics

Astronomy

Scientific paper

The Magdalena Ridge Observatory (MRO) project is presently funded to design and build a facility including an optical/infrared imaging interferometer composed of up to 10 1.5 meter class telescopes and a single conventional 2.4 meter class telescope. The interferometer array will be arranged in a “Y” configuration and the use of movable telescopes will allow its reconfiguration from a very compact array with baselines up to tens of meters to a true long baseline configuration with baselines up to 400 meters. We plan to introduce adaptive optics systems on the array telescopes.

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