Zobrazeno 1 - 10
of 20
pro vyhledávání: '"César Hernández‐Aguayo"'
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 1, p 126 (2024)
The statistical analysis of cosmic large-scale structure is most often based on simple two-point summary statistics, like the power spectrum or the two-point correlation function of a sample of galaxies or other types of tracers. In contrast, topolog
Externí odkaz:
https://doaj.org/article/25792d858e374508949fd654b6d68ea2
Autor:
Jiamin Hou, Julian Bautista, Maria Berti, Carolina Cuesta-Lazaro, César Hernández-Aguayo, Tilman Tröster, Jinglan Zheng
Publikováno v:
Universe, Vol 9, Iss 7, p 302 (2023)
The current standard cosmological model is constructed within the framework of general relativity with a cosmological constant Λ, which is often associated with dark energy, and phenomenologically explains the accelerated cosmic expansion. Understan
Externí odkaz:
https://doaj.org/article/43869c3954064341a4dbda87400c81eb
Publikováno v:
Astronomische Nachrichten. 344
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7d8489059cc8edeec3155baeebde6cc4
https://doi.org/10.1002/asna.20220110
https://doi.org/10.1002/asna.20220110
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2021, Vol.503(3), pp.3867-3885 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
We carry out ``full-physics'' hydrodynamical simulations of galaxy formation in the normal-branch Dvali-Gabadadze-Porrati (nDGP) braneworld model using a new modified version of the {\sc Arepo} code and the IllustrisTNG galaxy formation model. We sim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f5184fb2cea99e98bb847c2f5d521bd
https://doi.org/10.1093/mnras/stab694
https://doi.org/10.1093/mnras/stab694
Autor:
Cameron Grove, Chia-Hsun Chuang, Ningombam Chandrachani Devi, Lehman Garrison, Benjamin L’Huillier, Yu Feng, John Helly, César Hernández-Aguayo, Shadab Alam, Hanyu Zhang, Yu Yu, Shaun Cole, Daniel Eisenstein, Peder Norberg, Risa Wechsler, David Brooks, Kyle Dawson, Martin Landriau, Aaron Meisner, Claire Poppett, Gregory Tarlé, Octavio Valenzuela
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2022, Vol.515(2) [Peer Reviewed Journal]
Analysis of large galaxy surveys requires confidence in the robustness of numerical simulation methods. The simulations are used to construct mock galaxy catalogs to validate data analysis pipelines and identify potential systematics. We compare thre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96e6e0f23dbeff74241adde478f97e5d
http://arxiv.org/abs/2112.09138
http://arxiv.org/abs/2112.09138
Autor:
Cheng-Zong Ruan, Carolina Cuesta-Lazaro, Alexander Eggemeier, César Hernández-Aguayo, Carlton M Baugh, Baojiu Li, Francisco Prada
Publikováno v:
Monthly Notices of Royal Astronomical Society, 2022, Vol.514(1), pp.440-459 [Peer Reviewed Journal]
The coming generation of galaxy surveys will provide measurements of galaxy clustering with unprecedented accuracy and data size, which will allow us to test cosmological models at much higher precision than achievable previously. This means that we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::46e04ca98487e0ed54f476f9d923d739
http://arxiv.org/abs/2110.10033
http://arxiv.org/abs/2110.10033
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2019, Vol.485(2), pp.2194-2213 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
Measurements of redshift space distortions (RSD) provide a means to test models of gravity on large-scales. We use mock galaxy catalogues constructed from large N-body simulations of standard and modified gravity models to measure galaxy clustering i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c2a4703f264d1c8a1266fce0815766a
https://doi.org/10.1093/mnras/stz516
https://doi.org/10.1093/mnras/stz516
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=r3c4b2081b22::745ec781b416b687345dd858e347bc97
Publikováno v:
Monthly Notices of the Royal Astronomical Society.
We study and model the properties of galaxy clusters in the normal-branch Dvali-Gabadadze-Porrati (nDGP) model of gravity, which is representative of a wide class of theories which exhibit the Vainshtein screening mechanism. Using the first cosmologi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::745ec781b416b687345dd858e347bc97
https://doi.org/10.1093/mnras/stab2817
https://doi.org/10.1093/mnras/stab2817
Publikováno v:
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Monthly notices of the Royal Astronomical Society, 2021, Vol.503(2), pp.2318-2339 [Peer Reviewed Journal]
Digital.CSIC. Repositorio Institucional del CSIC
instname
Consejo Superior de Investigaciones Científicas (CSIC)
Monthly notices of the Royal Astronomical Society, 2021, Vol.503(2), pp.2318-2339 [Peer Reviewed Journal]
Digital.CSIC. Repositorio Institucional del CSIC
instname
Upcoming surveys will use a variety of galaxy selections to map the large-scale structure of the Universe. It is important to make accurate predictions for the properties and clustering of such galaxies, including the errors on these statistics. Here
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::980a3f6aef44c78251729b8eea733809
http://hdl.handle.net/10261/247862
http://hdl.handle.net/10261/247862