Pulsor observing system and data analysis procedure used at MRT

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4353

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DC Field	Value	Language
dc.contributor.author	Issur, N.H.	-
dc.contributor.author	Deshpande, A.A.	-
dc.date.accessioned	2012-02-15T10:05:18Z	-
dc.date.available	2012-02-15T10:05:18Z	-
dc.date.issued	2001	-
dc.identifier.citation	Tenth United Nations/European Sapce Agency Workshop on Basic Space science. Hosted by the University of Mauritius, 25-29 June 2001	en
dc.identifier.uri	http://hdl.handle.net/2289/4353	-
dc.description	Restricted Access	en
dc.description.abstract	The Mauritius Radio Telescope (MRT) was designed to operate mainly as an imaging instrument to carry out a southern sky survey at 150 MHz. However, it has also been successfully used it for pulsar observations. In this paper, we give an overview of the pulsar observing system we developed for use at MRT. Our pulsar receiver is of the 'direct-recording' type whereby most of the data processing, including dedispersion is done completely offline. The various steps involved in this data processing are also briefly described.	en
dc.language.iso	en	en
dc.rights	Raman Research Institute, Bangalore	en
dc.title	Pulsor observing system and data analysis procedure used at MRT	en
dc.type	Other	en
Appears in Collections:	Miscellaneous

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