Ten-meter radio telescope - A VLBI network element

Details Ten-meter radio telescope - A VLBI network element Ten-meter radio telescope - A VLBI network element

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..149d&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 149; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 4, April 1992, p. 39

Astronomy and Astrophysics

Astronomy

Radio Astronomy, Radio Telescopes, Very Long Base Interferometry, Heterodyning, Millimeter Waves, Radio Receivers

Scientific paper

A 10-m radio telescope of the Ranam Research Institute, Bangalore, India, has been equipped with a 22-GHz low-noise receiver, a coherent local oscillator, a hydrogen frequency standard, and an MK-2 terminal. The antenna's effective area is 50 sq m, and the system noise temperature is 60 K. VLBI observations of H2O maser sources were made in May 1990 at the Bangalore-EVN VLBI network. The angular sizes of the compact components and the coordinates of the radio telescope are determined.

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