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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.
Papers
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Journal ArticleDOI
The dependence of velocity and clustering statistics on galaxy properties
Andrew J. Benson,Carlton M. Baugh,Shaun Cole,Carlos S. Frenk,Cedric G. Lacey,Cedric G. Lacey +5 more
TL;DR: In this article, a combination of N-body simulations of the hierarchical clustering of dark matter and semi-analytic modelling of galaxy formation is used to probe the relationship between the galaxy distribution and the mass distribution in a flat, cold dark matter universe with mean density 0 = 0.3.
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The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos
Idit Zehavi,Sergio Contreras,Sergio Contreras,Nelson Padilla,Nicholas J. Smith,Nicholas J. Smith,Carlton M. Baugh,Peder Norberg +7 more
TL;DR: In this article, the dependence of the galaxy content of dark matter halos on large-scale environment and halo formation time using semi-analytic galaxy models applied to the Millennium simulation was studied.
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Which galaxies dominate the neutral gas content of the Universe
Claudia del P. Lagos,Carlton M. Baugh,Martin Zwaan,Cedric G. Lacey,Violeta Gonzalez-Perez,Chris Power,A. M. Swinbank,E. van Kampen +7 more
TL;DR: In this paper, the contribution of galaxies with different properties to the global densities of star formation rate (SFR), atomic (H)I and molecular hydrogen (H2) as a function of redshift was studied.
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Weak lensing by voids in modified lensing potentials
TL;DR: In this paper, the authors studied lensing by voids in the Cubic Galileon and Nonlocal gravity cosmologies, which are examples of theories of gravity that modify the lensing potential.
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Statistical Analysis of Galaxy Surveys-II. The 3-point galaxy correlation function measured from the 2dFGRS
TL;DR: In this paper, the authors present new results for the 3-point correlation function, measured as a function of scale, luminosity and colour from the final version of the two-degree field galaxy redshift survey (2dFGRS), employing a full covariance analysis.