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The mass of radio galaxies from low to high redshift

Abstract:
Using a new radio sample, 6C* designed to find radio galaxies at z > 4 along with the complete 3CRR and 6CE sample we extend the radio galaxy K-z relation to z~4.5. The 6C* K-z data significantly improve delineation of the K-z relation for radio galaxies at high redshift (z >2). In a spatially flat universe with a cosmological constant (Omega_M=0.3 and Omega_Lambda=0.7), the most luminous radio sources appear to be associated with galaxies with a luminosity distribution with a high mean (~5L*), and a low dispersion (~0.5 mag) which formed their stars at epochs corresponding to z >~ 2.5.
Publication status:
Published

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Publisher copy:
10.1007/10899892_36

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Journal:
MASS OF GALAXIES AT LOW AND HIGH REDSHIFT More from this journal
Pages:
148-153
Publication date:
2001-12-14
Event title:
Workshop on the Mass of Galaxies at Low and High Redshift
DOI:
ISBN:
3540002057


Keywords:
Pubs id:
pubs:29353
UUID:
uuid:0aa41168-5ee7-4929-8715-fca8719c169f
Local pid:
pubs:29353
Source identifiers:
29353
Deposit date:
2012-12-19
ARK identifier:

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