Mitaka optical/InfraRed Array, MIRA-I.2, has detected first stellar fringes on 30-m baseline

Details Mitaka optical/InfraRed Array, MIRA-I.2, has detected first stellar fringes on 30-m baseline Mitaka optical/InfraRed Array, MIRA-I.2, has detected first stellar fringes on 30-m baseline

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asthe..96..537o&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 96, No. 10, p. 537 - 545 (2003)

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Optical/Infrared Arrays

Scientific paper

On June 8, 2002, MIRA-I.2 (Mitaka optical/InfraRed Array I 2nd stage) observed first stellar fringes with Vega on 30-m baseline. The primary objective of MIRA-I.2 is to determine stellar diameter and mass accurately with its high angular resolution of a few mas. Currently, many optical and infrared interferometers, including MIRA-I.2, are under operation in the world. It is expected that exciting astronomical studies on stars and other celestial bodies, such as AGN and extra-solar planets, will be done using these interferometers in the near future. In this paper, we briefly introduce principles of interferometry and report current status of our optical interferometry.

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