Cosmological implications of a modified galaxy cluster pressure profile using the Planck tSZ power spectrum
The mean pressure profile of the cluster population is a key element in cosmological analyses based on surveys of galaxy clusters observed through the Sunyaev-Zel’dovich (SZ) effect. A variation of both the shape and the amplitude of this profile could explain part of the discrepancy currently obser...
Furkejuvvon:
| Váldodahkkit: | , , , |
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| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
EDP Sciences
2020-01-01
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| Ráidu: | EPJ Web of Conferences |
| Liŋkkat: | https://www.epj-conferences.org/articles/epjconf/pdf/2020/04/epjconf_mmuniverse2019_00025.pdf |
| Fáddágilkorat: |
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