We present a large-scale clustering analysis of radio galaxies in the Very Large Array Faint Images of the Radio Sky at Twenty-cm survey over the Galaxy and Mass Assembly (GAMA) survey area, limited to S1.4GHz > 1mJy with spectroscopic and photometric redshift limits up to r <19.8 and 1. This is indicative of an increasing (rather than fixed) halo mass and/or active galactic nuclei fraction at higher redshifts or a larger typical halo mass for the more abundant Fanaroff and Riley Class I sources. © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.
|Journal||Monthly Notices of the Royal Astronomical Society|
|Publication status||Published - 2014|