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http://hdl.handle.net/2289/5131
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DC Field | Value | Language |
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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) |
Files in This Item:
File | Description | Size | Format | |
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1992_Soviet Astronomy Letters_Vol.18_p149.pdf Restricted Access | Restricted Access | 528.46 kB | Adobe PDF | View/Open Request a copy |
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