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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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Secular evolution of galactic discs: constraints on phase-space density
TL;DR: In this paper, the phase-space density of the bulge of a galaxy was investigated using high-resolution N-body simulations. But the results showed that the size of the central regions is significantly larger than those in the inner parts of the galaxy.
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Full-sky photon simulation of clusters and active galactic nuclei in the soft X-rays for eROSITA
Johan Comparat,Dominique Eckert,Alexis Finoguenov,R. W. Schmidt,Jeremy S. Sanders,Daisuke Nagai,Erwin T. Lau,Florian Kaefer,Florian Pacaud,Nicolas Clerc,Thomas H. Reiprich,Esra Bulbul,Jacob Ider Chitham,Chia-Hsun Chuang,Vittorio Ghirardini,Violeta Gonzalez-Perez,Ghassem Gozaliazl,C. C. Kirkpatrick,Anatoly Klypin,Andrea Merloni,Kirpal Nandra,Teng Liu,Francisco Prada,Miriam E. Ramos-Ceja,Mara Salvato,R. Seppi,Elmo Tempel,Gustavo Yepes +27 more
TL;DR: In this article, a set of full sky light-cones using the MultiDark and UNIT dark matter only N-body simulations were created to predict the X-ray emission of galaxy clusters.
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The virialized mass of dark matter haloes
TL;DR: In this paper, the authors analyzed the properties of haloes of different masses focusing on the size of the region with zero mean radial velocity and found that the mass of this region is a much better approximation for the virial mass.
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Statistical Tests for CHDM and \LambdaCDM Cosmologies
TL;DR: In this paper, the authors apply several statistical estimators to high-resolution N-body simulations of two currently viable cosmological models: a mixed dark matter model, having $\Omega_
u=0.2$ contributed by two massive neutrinos (C+2
uDM), and a Cold Dark Matter model with Cosmological Constant (\LambdaCDM) with h = 0.3$ and h= 0.7.
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample
Sicheng Lin,Jeremy L. Tinker,Anatoly Klypin,Francisco Prada,Michael R. Blanton,Johan Comparat,Kyle S. Dawson,Arnaud de Mattia,Hélion du Mas des Bourboux,Will J. Percival,Will J. Percival,Anand Raichoor,Graziano Rossi,Alex Smith,Cheng Zhao +14 more
TL;DR: SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group and the French Participation Group.