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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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Radiative feedback and the low efficiency of galaxy formation in low-mass haloes at high redshift

TL;DR: In this article, the effect of radiation pressure in cosmological, zoom-in galaxy formation simulations is modeled as a non-thermal pressure that acts only in dense and optically thick star-forming regions.
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The AGORA High-Resolution Galaxy Simulations Comparison Project

TL;DR: AGORA as discussed by the authors is a comprehensive numerical study of well-resolved galaxies within the LCDM cosmology, which is run with a variety of code platforms to follow the hierarchical growth, star formation history, morphological transformation, and the cycle of baryons in and out of 8 galaxies with halo masses M_vir ~= 1.7e11, 1.1e10, 1e11 and 1e12.
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A Dynamical Classification of the Cosmic Web

TL;DR: In this article, a dynamical classification of the cosmic web is proposed, based on counting the number of eigenvalues above a certain threshold, lambda_th at each grid point, where the case of zero, one, two or three such eigen values corresponds to void, sheet, filament or a knot grid point.
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The MultiDark Database: Release of the Bolshoi and MultiDark Cosmological Simulations

TL;DR: The online MultiDark Database -- a Virtual Observatory-oriented, relational database for hosting various cosmological simulations is presented, which is further proof of the viability to store and present complex data using relational database technology.
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The structure of voids

TL;DR: In this paper, the authors used high-resolution N-body simulations to study the emptiness of giant 20h − 1 Mpc-diameter voids found in the distribution of bright galaxies.