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dc.contributor.authorJackson, C.
dc.contributor.authorFranzen, T.
dc.contributor.authorSeymour, N.
dc.contributor.authorWhite, S.
dc.contributor.authorMurphy, T.
dc.contributor.authorSadler, E.
dc.contributor.authorCallingham, J.
dc.contributor.authorHunstead, R.
dc.contributor.authorHughes, J.
dc.contributor.authorWall, J.
dc.contributor.authorBell, M.
dc.contributor.authorDwarakanath, K.
dc.contributor.authorFor, B.
dc.contributor.authorGaensler, B.
dc.contributor.authorHancock, P.
dc.contributor.authorHindson, L.
dc.contributor.authorHurley-Walker, N.
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorKapínska, A.
dc.contributor.authorLenc, E.
dc.contributor.authorMcKinley, B.
dc.contributor.authorMorgan, J.
dc.contributor.authorOffringa, A.
dc.contributor.authorProcopio, P.
dc.contributor.authorStaveley-Smith, L.
dc.contributor.authorWayth, Randall
dc.contributor.authorWu, C.
dc.contributor.authorZheng, Q.
dc.date.accessioned2017-01-30T13:40:23Z
dc.date.available2017-01-30T13:40:23Z
dc.date.created2016-10-09T19:30:47Z
dc.date.issued2015
dc.identifier.citationJackson, C. and Franzen, T. and Seymour, N. and White, S. and Murphy, T. and Sadler, E. and Callingham, J. et al. 2015. The MWA GLEAM 4 Jy sample; a new large, bright radio source sample at 151 MHz, in Conference Proceedings: The many facets of radio galaxies, Oct 20-23 2015. Bologna: POS.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/33942
dc.description.abstract

This paper outlines how the new GaLactic and Extragalactic All-sky MWA Survey (GLEAM, Wayth et al. 2015), observed by the Murchison Widefield Array covering the frequency range 72 231 MHz, allows identification of a new large, complete, sample of more than 2000 bright extragalactic radio sources selected at 151 MHz. With a flux density limit of 4 Jy this sample is significantly larger than the canonical fully-complete sample, 3CRR (Laing, Riley & Longair 1983). In analysing this small bright subset of the GLEAM survey we are also providing a firstuser check of the GLEAM catalogue ahead of its public release (Hurley-Walker et al. in prep). Whilst significant work remains to fully characterise our new bright source sample, in time it will provide important constraints to evolutionary behaviour, across a wide redshift and intrinsic radio power range, as well as being highly complementary to results from targeted, small area surveys.

dc.publisherSPIE - Internatioal Society for Optocal Engineering
dc.titleThe MWA GLEAM 4 Jy sample; a new large, bright radio source sample at 151 MHz
dc.typeJournal Article
dcterms.source.volume20-23-October-2015
dcterms.source.titleProceedings of Science
curtin.note

This open access article is distributed under the Creative Commons license http://creativecommons.org/licenses/by-nc-nd/4.0/

curtin.departmentDepartment of Electrical and Computer Engineering
curtin.accessStatusOpen access


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