Average dark matter halo sparsity relations as consistency check of mass estimates in galaxy cluster samples

Author:

Corasaniti Pier Stefano12,Rasera Yann1

Affiliation:

1. LUTH, UMR 8102 CNRS, Observatoire de Paris, PSL Research University, Université Paris Diderot, 5 Place Jules Janssen, F-92190 Meudon, France

2. Sorbonne Université, CNRS, UMR 7095, Institut d´Astrophysique de Paris, 98 bis bd Arago, F-75014 Paris, France

Funder

H2020 European Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 9 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. From inflation to dark matter halo profiles: the impact of primordial non-Gaussianities on the central density cusp;Journal of Cosmology and Astroparticle Physics;2024-05-01

2. X-ray Cluster Cosmology;Handbook of X-ray and Gamma-ray Astrophysics;2024

3. On the choice of the most suitable indicator for the assembly state of dark matter haloes through cosmic time;Monthly Notices of the Royal Astronomical Society;2023-01-10

4. X-Ray Cluster Cosmology;Handbook of X-ray and Gamma-ray Astrophysics;2023

5. Forecasting cosmological parameter constraints using multiple sparsity measurements as tracers of the mass profiles of dark matter haloes;Monthly Notices of the Royal Astronomical Society;2022-08-04

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