The MWA GLEAM 4 Jy sample; a new large, bright radio source sample at 151 MHz
dc.contributor.author | Jackson, C. | |
dc.contributor.author | Franzen, T. | |
dc.contributor.author | Seymour, N. | |
dc.contributor.author | White, S. | |
dc.contributor.author | Murphy, T. | |
dc.contributor.author | Sadler, E. | |
dc.contributor.author | Callingham, J. | |
dc.contributor.author | Hunstead, R. | |
dc.contributor.author | Hughes, J. | |
dc.contributor.author | Wall, J. | |
dc.contributor.author | Bell, M. | |
dc.contributor.author | Dwarakanath, K. | |
dc.contributor.author | For, B. | |
dc.contributor.author | Gaensler, B. | |
dc.contributor.author | Hancock, P. | |
dc.contributor.author | Hindson, L. | |
dc.contributor.author | Hurley-Walker, N. | |
dc.contributor.author | Johnston-Hollitt, M. | |
dc.contributor.author | Kapínska, A. | |
dc.contributor.author | Lenc, E. | |
dc.contributor.author | McKinley, B. | |
dc.contributor.author | Morgan, J. | |
dc.contributor.author | Offringa, A. | |
dc.contributor.author | Procopio, P. | |
dc.contributor.author | Staveley-Smith, L. | |
dc.contributor.author | Wayth, Randall | |
dc.contributor.author | Wu, C. | |
dc.contributor.author | Zheng, Q. | |
dc.date.accessioned | 2017-01-30T13:40:23Z | |
dc.date.available | 2017-01-30T13:40:23Z | |
dc.date.created | 2016-10-09T19:30:47Z | |
dc.date.issued | 2015 | |
dc.identifier.citation | Jackson, 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.uri | http://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.publisher | SPIE - Internatioal Society for Optocal Engineering | |
dc.title | The MWA GLEAM 4 Jy sample; a new large, bright radio source sample at 151 MHz | |
dc.type | Journal Article | |
dcterms.source.volume | 20-23-October-2015 | |
dcterms.source.title | Proceedings of Science | |
curtin.note |
This open access article is distributed under the Creative Commons license | |
curtin.department | Department of Electrical and Computer Engineering | |
curtin.accessStatus | Open access |