Molonglo deep survey at 843 MHZ

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4233

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DC Field	Value	Language
dc.contributor.author	Subrahmanya, C.R.	-
dc.contributor.author	Mills, B.Y.	-
dc.date.accessioned	2011-12-15T05:59:13Z	-
dc.date.available	2011-12-15T05:59:13Z	-
dc.date.issued	1987	-
dc.identifier.citation	Observational Cosmology; Proceedings of the IAU Symposium, Beijing, People's Republic of China, Aug. 25-30, 1986.	en
dc.identifier.uri	http://hdl.handle.net/2289/4233	-
dc.description	Restricted Access.	en
dc.description.abstract	The Molonglo Observatory Synthesis Telescope has been used for a deep survey of 25 southern fields of about 1° diameter. All these fields have been observed on several occasions in 120×12-hour sessions during 1983 - 85. Radio sources have thus been detected down to a few millijansky at 843 MHz in 20 deg2 of sky from these observations and in a few selected fields, it has been possible to reach a detection limit of 1 mJy. The first results on the source counts and optical identifications are presented. By supplementing these data with some existing observations of stronger radio sources, the authors have been able to obtain source counts at 843 MHz for the entire range of flux densities above 1 mJy.	en
dc.language.iso	en	en
dc.publisher	Dordrecht, D. Reidel Publishing Co.	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1987IAUS..124..569S	en
dc.rights	1987 Dordrecht, D. Reidel Publishing Co.	en
dc.title	Molonglo deep survey at 843 MHZ	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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