The Three Hundred Project: The evolution of galaxy cluster density profiles

Author:

Mostoghiu Robert1ORCID,Knebe Alexander123ORCID,Cui Weiguang1ORCID,Pearce Frazer R4,Yepes Gustavo12,Power Chris3,Dave Romeel5,Arth Alexander67

Affiliation:

1. Departamento de Física Teórica, Módulo 15, Facultad de Ciencias, Universidad Autónoma de Madrid, E-28049 Madrid, Spain

2. Centro de Investigación Avanzada en Física Fundamental (CIAFF), Facultad de Ciencias, Universidad Autónoma de Madrid, E-28049 Madrid, Spain

3. International Centre for Radio Astronomy Research, University of Western Australia, 35 Stirling Highway, Crawley, Western Australia 6009, Australia

4. School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, UK

5. Institute for Astronomy, School of Physics and Astronomy, The University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, UK

6. University Observatory Munich, Scheinerstraße 1, D-81679 Munich, Germany

7. Max-Planck-Institute for Extraterrestrial Physics, Giessenbachstrasse 1, D-85748 Garching, Germany

Funder

Horizon 2020

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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2. Euclid preparation;Astronomy & Astrophysics;2024-01

3. The impact of halo concentration on the Sunyaev Zel’dovich effect signal from massive galaxy clusters;Monthly Notices of the Royal Astronomical Society;2023-11-27

4. Modelling the mass accretion histories of dark matter haloes using a gamma formalism;Monthly Notices of the Royal Astronomical Society;2023-05-19

5. The Three Hundred Project: the evolution of physical baryon profiles;Monthly Notices of the Royal Astronomical Society;2023-05-18

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