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RT-10: A new element in the VLBI network

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dc.contributor.authorDhawan, V
dc.contributor.authorSarma, N V G
dc.contributor.authorGanesh, R
dc.contributor.authorMatveenko, L I
dc.contributor.authorKogan, L R
dc.contributor.authorMolodyanu, A P
dc.contributor.authorGraham, D A
dc.date.accessioned2012-08-03T05:46:11Z
dc.date.available2012-08-03T05:46:11Z
dc.date.issued1992
dc.descriptionRestricted Access.en
dc.description.abstractA 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.en
dc.identifier.citationSoviet Astronomy Letters, 1992, Vol.18, p149en
dc.identifier.issn0360-0327
dc.identifier.urihttp://hdl.handle.net/2289/5131
dc.language.isoenen
dc.publisherAstrophysical Data Serviceen
dc.relation.urihttp://adsabs.harvard.edu/abs/1992SvAL...18..149Den
dc.rights1992 American Institute of Physicsen
dc.subjectradio astronomyen
dc.subjectradio telescopesen
dc.subjectvery long base interferometryen
dc.subjectheterodyningen
dc.subjectmillimeter wavesen
dc.subjectradio receiversen
dc.titleRT-10: A new element in the VLBI networken
dc.typeArticleen

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