Galaxy and mass assembly: The evolution of bias in the radio source population to z ~ 1.5

S.N. Lindsay, M.J. Jarvis, M.G. Santos, M.J.I. Brown, S.M. Croom, Simon Driver, A.M. Hopkins, J. Liske, J.N. Loveday, P. Norberg, Aaron Robotham

    Research output: Contribution to journalArticle

    27 Citations (Scopus)
    148 Downloads (Pure)

    Abstract

    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.
    Original languageEnglish
    Pages (from-to)1527-1541
    JournalMonthly Notices of the Royal Astronomical Society
    Volume440
    Issue number2
    DOIs
    Publication statusPublished - 2014

    Fingerprint Dive into the research topics of 'Galaxy and mass assembly: The evolution of bias in the radio source population to z ~ 1.5'. Together they form a unique fingerprint.

  • Cite this

    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