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.
Lindsay, S. N., Jarvis, M. J., Santos, M. G., Brown, M. J. I., Croom, S. M., Driver, S., Hopkins, A. M., Liske, J., Loveday, J. N., Norberg, P., & Robotham, A. (2014). Galaxy and mass assembly: The evolution of bias in the radio source population to z ~ 1.5. Monthly Notices of the Royal Astronomical Society, 440(2), 1527-1541. https://doi.org/10.1093/mnras/stu354