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This paper outlines how the new GaLactic and Extragalactic All-sky MWA Survey(GLEAM, Wayth et al. 2015), observed by the Murchison Widefield Array coveringthe frequency range 72 - 231 MHz, allows identification of a new large,complete, sample of more than 2000 bright extragalactic radio sources selectedat 151 MHz. With a flux density limit of 4 Jy this sample is significantlylarger than the canonical fully-complete sample, 3CRR (Laing, Riley & Longair1983). In analysing this small bright subset of the GLEAM survey we are alsoproviding a first user check of the GLEAM catalogue ahead of its public release(Hurley-Walker et al. in prep). Whilst significant work remains to fullycharacterise our new bright source sample, in time it will provide importantconstraints to evolutionary behaviour, across a wide redshift and intrinsicradio power range, as well as being highly complementary to results fromtargeted, small area surveys.

The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz