  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 first user 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.
