Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/942
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Sukumar, S et. al. | - |
dc.date.accessioned | 2006-04-11T08:08:00Z | - |
dc.date.available | 2006-04-11T08:08:00Z | - |
dc.date.issued | 1988 | - |
dc.identifier.citation | BASI, Vol. 16, No. 2 & 3, pp. 93-110 | en |
dc.identifier.uri | http://hdl.handle.net/2248/942 | - |
dc.description.abstract | The principle, design and operational parameters of the Ooty synthesis radio telescope (OSRT) are described. It consists of thirteen elements including the Ooty Radio Telescope, which is divided into five parts. Operating at 327 MHz OSRT provides a resolution of about 36 x 60 arcsec and a sensitivity of about 4 mJy for 9 hours of observation | en |
dc.format.extent | 1653046 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of Indian | en |
dc.subject | Radio astronomy | en |
dc.subject | Aperture synthesis | en |
dc.title | Ooty synthesis radio telescope - Design and performance | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
SUKUMAR.pdf | 1.61 MB | Adobe PDF | ![]() View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.