The Murchison widefield array

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4240

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DC Field	Value	Language
dc.contributor.author	Mitchell, D.A.	-
dc.contributor.author	Gopalakrishna, M.R.	-
dc.contributor.author	Kamini, P.A.	-
dc.contributor.author	Madhavi, S.	-
dc.contributor.author	Prabu, T.	-
dc.contributor.author	Udaya Shankar, N.	-
dc.date.accessioned	2011-12-21T05:17:04Z	-
dc.date.available	2011-12-21T05:17:04Z	-
dc.date.issued	2010-03	-
dc.identifier.citation	Proceedings of Science, 2010, RFI2010, p016	en
dc.identifier.issn	1824-8039	-
dc.identifier.uri	http://hdl.handle.net/2289/4240	-
dc.description	Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)	en
dc.description.abstract	It is shown that the excellent Murchison Radio-astronomy Observatory site allows the Murchison Widefield Array to employ a simple RFI blanking scheme and still calibrate visibilities and form images in the FM radio band. The techniques described are running autonomously in our calibration and imaging software, which is currently being used to process an FM-band survey of the entire southern sky.	en
dc.language.iso	en	en
dc.publisher	SISSA	en
dc.relation.uri	http://arxiv.org/abs/1008.2551	en
dc.rights	Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.	en
dc.title	The Murchison widefield array	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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