Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters
The gas mass fraction in galaxy clusters is a quantity which can be used as a robust cosmological probe. It is however subject to various effects from the baryonic physics inside galaxy clusters, which may bias the obtained cosmological constraints. Among different aspects of the baryonic physics, i...
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| Hlavní autoři: | , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
EDP Sciences
2024-01-01
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| Edice: | EPJ Web of Conferences |
| On-line přístup: | https://www.epj-conferences.org/articles/epjconf/pdf/2024/03/epjconf_mmUniverse2023_00052.pdf |
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