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Journal article

The clustering and bias of radio-selected AGN and star-forming galaxies in the COSMOS field

Abstract:

Dark matter haloes in which galaxies reside are likely to have a significant impact on their evolution. We investigate the link between dark matter haloes and their constituent galaxies by measuring the angular two-point correlation function of radio sources, using recently released 3 GHz imaging over $\sim 2 \ \mathrm{deg}^2$ of the COSMOS field. We split the radio source population into Star Forming Galaxies (SFGs) and Active Galactic Nuclei (AGN), and further separate the AGN into radiativ...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/stx2954

Authors


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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
St Cross College
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Atomic and Laser Physics
Role:
Author
More from this funder
Name:
Seventh Framework program
Grant:
337595
More from this funder
Name:
Science and Technology Facilities Council
Grant:
ST/N000919/1
More from this funder
Name:
Hintze Family Charitable Foundation
More from this funder
Name:
Square Kilometre Array South Africa
Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
474
Issue:
3
Pages:
4133–4150
Publication date:
2017-11-01
Acceptance date:
2017-11-13
DOI:
Keywords:
Pubs id:
pubs:809882
UUID:
uuid:625fe377-0c77-4f86-8b4a-aa0cb5a37a5c
Local pid:
pubs:809882
Source identifiers:
809882
Deposit date:
2018-01-11

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