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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 journey of QSO haloes from z ∼ 6 to the present
Raul E. Angulo,Volker Springel,Volker Springel,Stephen White,Shaun Cole,Adrian Jenkins,Carlton M. Baugh,Carlos S. Frenk +7 more
TL;DR: In this paper, the authors apply a scaling technique to the Millennium-XXL, one of the largest cosmological N-body simulations carried out to date (3 × 1011 particles within a cube of volume ∼70 Gpc3).
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Marked clustering statistics in f(R) gravity cosmologies
TL;DR: In this paper, the two-point and marked correlation functions (mCFs) of haloes and galaxies in three variants of the chameleon f(R) gravity model using N-body simulations were compared to a fiducial Λ cold dark matter model based on general relativity (GR).
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Growing a "cosmic beast": observations and simulations of MACS J0717.5+3745
Mathilde Jauzac,Dominique Eckert,Matthieu Schaller,J. Schwinn,Richard Massey,Yannick M. Bahé,Yannick M. Bahé,Carlton M. Baugh,David J. Barnes,David J. Barnes,C. Dalla Vecchia,C. Dalla Vecchia,Harald Ebeling,David Harvey,Eric Jullo,Scott T. Kay,Jean-Paul Kneib,Jean-Paul Kneib,Marceau Limousin,Elinor Medezinski,Priyamvada Natarajan,Mario Nonino,Andrew Robertson,Sut-Ieng Tam,Keiichi Umetsu +24 more
TL;DR: In this article, the core of a massive galaxy cluster and its surrounding structures are analyzed using a gravitational lensing and X-ray analysis, and the authors find that the smooth accretion of surrounding material remains the main source of mass growth even for such massive clusters.
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No evidence for modifications of gravity from galaxy motions on cosmological scales
TL;DR: In this paper, a forward-modeling approach that fully exploits the sensitivity of the galaxy velocity field to modifications of general relativity (GR) has been proposed for galaxy clustering on cosmological scales.
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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 paper, 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.