Pulsar observations at 150 MHz with Mauritius Radio Telescope - Preliminary results

dc.contributor.author	Issur, N. H
dc.date.accessioned	2008-05-21T09:24:01Z
dc.date.available	2008-05-21T09:24:01Z
dc.date.issued	1997
dc.identifier.citation	BASI, Vol. 25, No. 4, pp. 541 - 548	en
dc.identifier.uri	http://hdl.handle.net/2248/2331
dc.description.abstract	The Mauritius Radio Telescope (MRT) has been used to observe some Southern Hemisphere pulsars at 151.6 MHz. A tracking system allowing observation of a source for 8 x sec (δ) minutes of time and a Fast Data Acquisition System were added to MRT in July 1996, for this purpose. With this new system, it is now possible to observe pulsars with an average flux density of about 100 mJy (with a signal to noise ratio of = 25). In this paper we describe the observations made with the new set up and report our preliminary results on 3 pulsars, including the bright millisecond pulsar J0437-4715.	en
dc.format.extent	510131 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1997BASI...25..541I	en
dc.subject	Pulsars	en
dc.subject	Millisecond Pulsar	en
dc.subject	Mauritius Radio Telescope	en
dc.title	Pulsar observations at 150 MHz with Mauritius Radio Telescope - Preliminary results	en
dc.type	Article	en