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

doi:10.1093/mnras/stu354

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

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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 language	English
Pages (from-to)	1527-1541
Journal	Monthly Notices of the Royal Astronomical Society
Volume	440
Issue number	2
DOIs	https://doi.org/10.1093/mnras/stu354
Publication status	Published - 2014

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10.1093/mnras/stu354

MNRAS-2014-Lindsay-1527-41
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved
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title = "Galaxy and mass assembly: The evolution of bias in the radio source population to z ~ 1.5",

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. {\textcopyright} 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.",

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

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T1 - Galaxy and mass assembly: The evolution of bias in the radio source population to z ~ 1.5

AU - Lindsay, S.N.

AU - Jarvis, M.J.

AU - Santos, M.G.

AU - Brown, M.J.I.

AU - Croom, S.M.

AU - Driver, Simon

AU - Hopkins, A.M.

AU - Liske, J.

AU - Loveday, J.N.

AU - Norberg, P.

AU - Robotham, Aaron

PY - 2014

Y1 - 2014

N2 - 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.

AB - 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.

U2 - 10.1093/mnras/stu354

DO - 10.1093/mnras/stu354

M3 - Article

VL - 440

SP - 1527

EP - 1541

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 2

ER -

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

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