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.
Original language | English |
---|---|
Title of host publication | Proceedings of Science |
Place of Publication | Italy |
Publisher | Proceedings of Science (PoS) |
Pages | 1-8 |
Volume | N/A |
Publication status | Published - 2015 |
Event | The many facets of extragalactic radio surveys: towards new scientific challenges - CRN Research Area, 101 Via Gobetti, Bologna, Italy Duration: 20 Oct 2015 → 23 Oct 2015 Conference number: 123437 https://pos.sissa.it/267/ |
Conference
Conference | The many facets of extragalactic radio surveys |
---|---|
Abbreviated title | EXTRA-RADSUR2015 |
Country/Territory | Italy |
City | Bologna |
Period | 20/10/15 → 23/10/15 |
Internet address |