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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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Constraining structure formation using EDGES
TL;DR: In this paper, a thermal warm dark matter (WDM) model with mass 4.3 was used to detect the 21-cm absorption line at 78MHz in the sky-averaged spectrum.
Journal ArticleDOI
Constraining structure formation using EDGES
TL;DR: In this article, the authors combine simulations of structure formation with a simple recipe for star formation to investigate whether these models emit enough Lyman-α photons to reproduce the experimental signal for reasonable values of the star formation efficiency.
Journal ArticleDOI
The morphological evolution of galaxy satellites
TL;DR: In this article, the evolution of galaxy satellites with high-resolution N-body simulations is studied, where the satellites are modeled as replicas of typical low and high surface brightness galaxies (LSBs and HSBs).
Posted Content
Distant monsters: high redshift AGN predictions from a $\Lambda$CDM cosmological model
Andrew J. Griffin,Cedric G. Lacey,Violeta Gonzalez-Perez,Claudia del P. Lagos,Carlton M. Baugh,N. Fanidakis +5 more
TL;DR: In this paper, an updated model for the evolution of masses and spins of supermassive black holes (SMBHs), coupled with the latest version of the semi-analytical model of galaxy formation GALFORM using the Planck cosmology and a high resolution Millennium style dark matter simulation to make predictions for AGN and SMBH properties for $0 < z < 6.
Cosmological Parameters 2006
TL;DR: In this article, the authors compare the constraints derived from the extant CMB data circa 2005 and the final 2dFGRS galaxy power spectrum, with the results obtained when the WMAP 1-year data is replaced by the 3-year measurements (hereafter WMAP1 and WMAP3).