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Anatoly Klypin
Researcher at New Mexico State University
Publications - 291
Citations - 42755
Anatoly Klypin is an academic researcher from New Mexico State University. The author has contributed to research in topics: Dark matter & Galaxy. The author has an hindex of 94, co-authored 287 publications receiving 40171 citations. Previous affiliations of Anatoly Klypin include University of Oxford & Spanish National Research Council.
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Journal ArticleDOI
The Relation Between Galaxy ISM and Circumgalactic OVI Gas Kinematics Derived from Observations and $\Lambda$CDM Simulations
Glenn G. Kacprzak,Jacob R. Vander Vliet,Nikole M. Nielsen,Sowgat Muzahid,Stephanie K. Pointon,Christopher W. Churchill,Daniel Ceverino,Kenz S. Arraki,Anatoly Klypin,Jane C. Charlton,James R. Lewis +10 more
TL;DR: In this paper, the authors present the first galaxy-OVI absorption kinematic study for 20 absorption systems associated with isolated galaxies (EW>0.15$ 33^{\circ}$).
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The dependence of halo bias on age, concentration, and spin
TL;DR: GSP and ADMD thank FAPESP for financial support. FP acknowledges support from the Spanish MINECO grant AYA2010-21231-C02-01 as mentioned in this paper.
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Tracing the nature of dark energy with galaxy distribution
TL;DR: In this article, the authors explore tests based on the galaxy mass function, the void probability function (VPF), and the number of galaxy clusters, and find that detecting a model dependence in the cluster redshift distribution is a significant challenge.
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Sizes of Voids as a Test for Dark Matter Models
Sebastiano Ghigna,Stefano Borgani,Silvio A. Bonometto,Luigi Guzzo,Anatoly Klypin,Joel R. Primack,Riccardo Giovanelli,Martha P. Haynes +7 more
TL;DR: In this paper, the authors compare observational results with theoretical predictions based on high-resolution N{body simulations for two realizations of the Cold+Hot Dark Matter (CHDM) model and for unbiased (b = 1) and biased (b < 1:5) CDM models in a 50 h 1Mpc box.
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The evolution of X-ray clusters in a cold plus hot dark matter universe
TL;DR: In this paper, the authors present the first self-consistently computed results on the evolution of X-ray properties of galaxy clusters in a cold + hot dark matter (CHDM) model.