C
C. M. Booth
Researcher at University of Chicago
Publications - 63
Citations - 9720
C. M. Booth is an academic researcher from University of Chicago. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 38, co-authored 63 publications receiving 8713 citations. Previous affiliations of C. M. Booth include Leiden University & Durham University.
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Journal ArticleDOI
The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
Joop Schaye,Robert A. Crain,Richard G. Bower,Michelle Furlong,Matthieu Schaller,Tom Theuns,Tom Theuns,Claudio Dalla Vecchia,Claudio Dalla Vecchia,Carlos S. Frenk,Ian G. McCarthy,John C. Helly,Adrian Jenkins,Yetli Rosas-Guevara,Simon D. M. White,Maarten Baes,C. M. Booth,C. M. Booth,Peter Camps,Julio F. Navarro,Yan Qu,Alireza Rahmati,Till Sawala,Peter A. Thomas,James W. Trayford +24 more
TL;DR: The Virgo Consortium's EAGLE project as discussed by the authors is a suite of hydrodynamical simulations that follow the formation of galaxies and black holes in representative volumes, where thermal energy is injected into the gas, allowing winds to develop without predetermined speed or mass loading factors.
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Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
C. M. Booth,Joop Schaye +1 more
TL;DR: In this article, Springel, Di Matteo & Hernquist present a method that self-consistently tracks the growth of supermassive black holes and the feedback from active galactic nuclei (AGN) in cosmological, hydrodynamical simulations.
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The physics driving the cosmic star formation history
Joop Schaye,Claudio Dalla Vecchia,C. M. Booth,Robert P. C. Wiersma,Tom Theuns,Tom Theuns,M.R. Haas,Serena Bertone,Alan R. Duffy,Alan R. Duffy,Ian G. McCarthy,Freeke van de Voort +11 more
TL;DR: In this paper, the authors investigate the physics driving the cosmic star formation history using the more than 50 large, cosmological, hydrodynamical simulations that together comprise the OverWhelmingly Large Simulations project.
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The effects of galaxy formation on the matter power spectrum: a challenge for precision cosmology
TL;DR: In this paper, the authors employed the large suite of simulations from the OverWhelmingly Large Simulations (OWLS) project to investigate the effects of various baryonic processes on the matter power spectrum.
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The case for AGN feedback in galaxy groups
Ian G. McCarthy,Joop Schaye,Trevor J. Ponman,Richard G. Bower,C. M. Booth,C. Dalla Vecchia,Robert A. Crain,Volker Springel,Tom Theuns,Tom Theuns,Robert P. C. Wiersma +10 more
TL;DR: In this article, the effects of supermassive black hole feedback on the star formation rate (SFRs) of galaxies was examined, and it was shown that BH feedback significantly reduced the gas mass fractions of galaxy groups with masses less than a few times 10 14 M�, yielding a gas mass fraction and X-ray luminosity scaling with system temperature that is in excellent agreement with the data, although the detailed scatter in the L T relation is not quite correct.