Phase-coherent astrometric interferometry

Details Phase-coherent astrometric interferometry Phase-coherent astrometric interferometry

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mit..reptw....s&link_type=abstract

Annual Report, 1 Feb. 1986 - 31 Jan. 1987 Massachusetts Inst. of Tech., Cambridge. Research Lab. of Electronics.

Astronomy and Astrophysics

Astronomy

Astrometry, Laser Interferometry, Michelson Interferometers, High Resolution, Kalman Filters, Pointing Control Systems, Star Trackers

Scientific paper

This year involved continuation of the development of the Mark III stellar interferometer, which is a fringe-tracking long-baseline Michelson interferometer designed primarily for wide-angle astrometry at the milli-arcsecond level. It also is useful for measuring stellar diameters and as an initial test bed for concepts relevant to aperture synthesis imaging. It is being constructed on Mount Wilson, California.

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