The first of these interferometers was the 20 foot Stellar Interferometer.
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The "'Michelson stellar interferometer "'is one of the earliest astronomical interferometers built and used.
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A high-precision orbit was published in 1994 based on observations by the Mark III Stellar Interferometer, again at Mount Wilson Observatory.
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The "'Sydney University Stellar Interferometer "'( SUSI ) is an optical long baseline interferometer owned by The University of Sydney.
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In observations made from 1990 to 1992, Eta Andromedae was resolved interferometrically by the Mark III Stellar Interferometer at Mount Wilson Observatory, California, United States.
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Notable 1990s results included the NPOI producing many very high resolution images, and Infrared Stellar Interferometer measurements of stars in the mid-infrared for the first time.
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The "'Palomar Testbed Interferometer "'( PTI ) was a near infrared, long-baseline stellar interferometer located at Palomar Observatory in north San Diego County, California, United States.
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One such example includes stellar interferometers in which multiple apertures, in controlled formation, collect the light for coherent interferometric beam combinations, thereby achieving a fine angular resolution comparable to a large monolithic aperture telescope.
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