Cosmology with the SZ spectrum: Measuring the Universe’s temperature with galaxy clusters
The hot gas in clusters of galaxies creates a distinctive spectral distortion in the cosmic microwave background (CMB) via the Sunyaev-Zel’dovich (SZ) effect. The spectral signature of the SZ can be used to measure the CMB temperature at cluster redshift (TCMB(z)) and to constrain the monopole of th...
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| Principais autores: | , , , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
EDP Sciences
2022-01-01
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| Series: | EPJ Web of Conferences |
| Acceso en liña: | https://www.epj-conferences.org/articles/epjconf/pdf/2022/01/epjconf_mmUniverse2021_00028.pdf |
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