The Smithsonian Astrophysical Observatory submillimeter wave telescope array

Details The Smithsonian Astrophysical Observatory submillimeter wave telescope array The Smithsonian Astrophysical Observatory submillimeter wave telescope array

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990liaco..29..161m&link_type=abstract

In ESA, From Ground-Based to Space-Borne Sub-mm Astronomy p 161-164 (SEE N91-21986 13-89)

Astronomy and Astrophysics

Astrophysics

Astrophysics, Radio Telescopes, Submillimeter Waves, Very Long Base Interferometry, Very Long Baseline Array (Vlba), Astronomical Observatories, Line Spectra, Spectrometers, Spectrum Analysis

Scientific paper

A submillimeter wavelength interferometer array built by the Smith Astrophysical Observatory is described. The telescope is to be located at a high mountain site and will operate in the major atmospheric windows from 200 to 900 GHz. The array is to consist of six antennas, each 6 m in diameter. All antennas are to be movable over a Y shaped track with maximum baselines of several hundred meters. The facility is designed to operate simultaneously at two different frequencies, and is equipped with a versatile digital spectrometer permitting measurements of many different lines at once.

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