RT-10: A new element in the VLBI network

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/5131

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DC Field	Value	Language
dc.contributor.author	Dhawan, V.	-
dc.contributor.author	Sarma, N.V.G.	-
dc.contributor.author	Ganesh, R.	-
dc.contributor.author	Matveenko, L.I.	-
dc.contributor.author	Kogan, L.R.	-
dc.contributor.author	Molodyanu, A.P.	-
dc.contributor.author	Graham, D.A.	-
dc.date.accessioned	2012-08-03T05:46:11Z	-
dc.date.available	2012-08-03T05:46:11Z	-
dc.date.issued	1992	-
dc.identifier.citation	Soviet Astronomy Letters, 1992, Vol.18, p149	en
dc.identifier.issn	0360-0327	-
dc.identifier.uri	http://hdl.handle.net/2289/5131	-
dc.description	Restricted Access.	en
dc.description.abstract	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.	en
dc.language.iso	en	en
dc.publisher	Astrophysical Data Service	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1992SvAL...18..149D	en
dc.rights	1992 American Institute of Physics	en
dc.subject	radio astronomy	en
dc.subject	radio telescopes	en
dc.subject	very long base interferometry	en
dc.subject	heterodyning	en
dc.subject	millimeter waves	en
dc.subject	radio receivers	en
dc.title	RT-10: A new element in the VLBI network	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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