Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3262
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dc.contributor.authorGolap, K-
dc.contributor.authorShankar, N. U-
dc.contributor.authorSachdev, S-
dc.contributor.authorDodson, R-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-08-22T11:15:02Z-
dc.date.available2008-08-22T11:15:02Z-
dc.date.issued1998-06-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 19, No. 1 - 2, pp. 35 - 53en
dc.identifier.issn0250 - 6335-
dc.identifier.urihttp://hdl.handle.net/2248/3262-
dc.description.abstractA new, meter-wave radio telescope has been built in the north-east of Mauritius, an island in the Indian Ocean, at a latitude of -20.14°. The Maritius Radio Telescope is a Fourier Synthesis T-shaped array, consisting of a 2048 m long East-West arm and an 800 m long South arm. The primary objective of the telkescope is to produce a sky survey in the declination range -70° to -10° with a point source sensitivity of about 200 mJy. This will be the southern sky equivalent of the Cambridge 6C survey. The authors describe the telescope, discuss the array design and the calibration techniques used, and present a map made using the telescope.en
dc.format.extent1706200 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1998JApA...19...35Gen
dc.subjectRadio Telescopesen
dc.subjectSky Surveysen
dc.titleA low frequency radio telescope at Mauritius for a southern sky survey.en
dc.typeArticleen
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