Euclid: Constraints on f(R) cosmologies from the spectroscopic and photometric primary probes★
We forecast the constraints that the Euclid mission will place on the Hu–Sawicki f(R) modified gravity model using galaxy clustering and weak lensing observations. Euclid’s primary probes will provide spectroscopic redshifts, photometric angular clustering, and weak lensing cosmic shear, thus allowi...
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| Autors principals: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
EDP Sciences
2026-03-01
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| Col·lecció: | Astronomy & Astrophysics |
| Matèries: | |
| Accés en línia: | https://www.aanda.org/articles/aa/full_html/2026/03/aa48713-23/aa48713-23.html |
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