Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/5131| Title: | RT-10: A new element in the VLBI network |
| Authors: | Dhawan, V. Sarma, N.V.G. Ganesh, R. Matveenko, L.I. Kogan, L.R. Molodyanu, A.P. Graham, D.A. |
| Keywords: | radio astronomy radio telescopes very long base interferometry heterodyning millimeter waves radio receivers |
| Issue Date: | 1992 |
| Publisher: | Astrophysical Data Service |
| Citation: | Soviet Astronomy Letters, 1992, Vol.18, p149 |
| 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. |
| Description: | Restricted Access. |
| URI: | http://hdl.handle.net/2289/5131 |
| ISSN: | 0360-0327 |
| Alternative Location: | http://adsabs.harvard.edu/abs/1992SvAL...18..149D |
| Copyright: | 1992 American Institute of Physics |
| Appears in Collections: | Research Papers (A&A) |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 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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