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Carlton M. Baugh
Researcher at Durham University
Publications - 482
Citations - 53635
Carlton M. Baugh is an academic researcher from Durham University. The author has contributed to research in topics: Galaxy & Galaxy formation and evolution. The author has an hindex of 110, co-authored 476 publications receiving 51655 citations. Previous affiliations of Carlton M. Baugh include University of Oxford & Illinois Central College.
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Journal ArticleDOI
The 2dF Galaxy Redshift Survey: the blue galaxy fraction and implications for the Butcher—Oemler effect
Roberto De Propris,Matthew Colless,John A. Peacock,Warrick J. Couch,Simon P. Driver,Michael L. Balogh,Ivan K. Baldry,Carlton M. Baugh,Joss Bland-Hawthorn,Terry J. Bridges,Russell D. Cannon,Shaun Cole,Chris A. Collins,Nicholas Cross,Gavin Dalton,Gavin Dalton,George Efstathiou,Richard S. Ellis,Carlos S. Frenk,Karl Glazebrook,Ed Hawkins,Carole Jackson,Ofer Lahav,Ian Lewis,Stuart Lumsden,Stephen J. Maddox,Darren Madgwick,Peder Norberg,Will J. Percival,Bruce A. Peterson,William J. Sutherland,Keith Taylor +31 more
TL;DR: In this article, the authors derived the fraction of blue galaxies in a sample of clusters at z < 0.11 and the general field at the same redshift and showed that the value of the blue fraction is observed to depend on the luminosity limit adopted, cluster-centric radius and, more generally, local galaxy density, but does not depend on cluster properties.
Journal ArticleDOI
The effects of photoionization on galaxy formation — III. Environmental dependence in the luminosity function
TL;DR: In this article, the authors calculate the luminosity function of galaxy populations residing in cold dark matter halos of different masses, and find substantial differences in the shapes of the galaxy luminosity functions in haloes of different mass, which reflect generic features of the cold-dark matter model of galaxy formation.
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Where are the stars
TL;DR: In this article, the authors used the Two-degree Field Galaxy Redshift Survey (2dFGRS) and the Two Micron All-Sky Survey (XSC) to study the near-infrared light and stellar mass content of the local Universe.
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The most luminous quasars do not live in the most massive dark matter haloes at any redshift
TL;DR: In this article, the authors show that in a galaxy formation model which includes AGN feedback, QSOs are predicted to live in DM haloes with typical masses of a few times 1012 M⊙.
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The properties of Lyα emitting galaxies in hierarchical galaxy formation models
TL;DR: In this paper, the authors present detailed predictions for the properties of Lyα-emitting galaxies in the framework of the Λ cold dark matter cosmology, calculated using the semi-analytical galaxy formation model galform.