Statistical characteristics of observed and simulated dark matter haloes-Reference-Cited by-同舟云学术

Statistical characteristics of observed and simulated dark matter haloes

Published:2023-08-21 Issue:2 Volume:525 Page:1922-1927
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Demiański M¹²^ORCID,Doroshkevich A³⁴,Larchenkova T³,Pilipenko S³

Affiliation:

1. Institute of Theoretical Physics, University of Warsaw , PL-02-093 Warsaw, Poland

2. Department of Astronomy , Williams College, Williamstown, MA 01267, USA

3. Lebedev Physical Institute of Russian Academy of Sciences , 119333 Moscow, Russian Federation, Russia

4. National Research Center Kurchatov Institute , 123182, Moscow, Russian Federation, Russia

Abstract

ABSTRACT A simple model of spherical dark matter haloes is proposed in terms of two structure functions. In the framework of this model, we analysed the properties of 450 000 simulated haloes with masses Mvir > 1011 M⊙. We compared the mean characteristics of simulated haloes with the corresponding characteristics of 641 galaxies and found that the basic characteristics of the two populations are similar but that their probability distribution functions are different. This disagreement may be caused by technical factors such as the halo identification algorithm, which does not reproduce the observed dark matter haloes correctly.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://academic.oup.com/mnras/article-pdf/525/2/1922/51236817/stad2349.pdf

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