Zobrazeno 1 - 10
of 173
pro vyhledávání: '"Anatoly Klypin"'
Publikováno v:
The Astrophysical Journal, Vol 955, Iss 1, p 26 (2023)
The cluster mass–richness relation (MRR) is an observationally efficient and potentially powerful cosmological tool for constraining the matter density Ω _m and the amplitude of fluctuations σ _8 using the cluster abundance technique. We derive t
Externí odkaz:
https://doaj.org/article/2a4edd23f9e94ee6899da607dc72c83d
Autor:
Johan Comparat, Dominique Eckert, Alexis Finoguenov, Robert Schmidt, Jeremy S. Sanders, Daisuke Nagai, Erwin T. Lau, Florian Käfer, Florian Pacaud, Nicolas Clerc, Thomas H. Reiprich, Esra Bulbul, Jacob Ider Chitham, Chia-Hsun Chiang, Vittorio Ghirardini, Violeta Gonzalez-Perez, Ghassem Gozaliasl, Charles C. Fitzpatrick, Anatoly Klypin, Andrea Merloni, Kirpal Nandra, Teng Liu, Francisco Prada, Miriam Ramos-Ceja, Marra Salvato, Riccardo Seppi, Elmo Tempel, Gustavo Yepes
Publikováno v:
The Open Journal of Astrophysics, Vol 3, Iss 1 (2020)
Externí odkaz:
https://doaj.org/article/5594a79c95bf4e439de37f564b783576
Autor:
Han Aung, Daisuke Nagai, Anatoly Klypin, Peter Behroozi, Mohamed H Abdullah, Tomoaki Ishiyama, Francisco Prada, Enrique Pérez, Javier López Cacheiro, José Ruedas
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 519:1648-1656
We present the public data release of the Uchuu-UM galaxy catalogues by applying the UNIVERSEMACHINE algorithm to assign galaxies to the dark matter haloes in the Uchuu N-body cosmological simulation. It includes a variety of baryonic properties for
Autor:
Kyle S. Dawson, Sicheng Lin, Michael R. Blanton, Will J. Percival, Johan Comparat, Jeremy L. Tinker, Graziano Rossi, Francisco Prada, Anand Raichoor, Hélion du Mas des Bourboux, Anatoly Klypin, Cheng Zhao, Alex Smith, Arnaud de Mattia
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 498 (4), pp.5251-5262. ⟨10.1093/mnras/staa2571⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 498 (4), pp.5251-5262. ⟨10.1093/mnras/staa2571⟩
Monthly Notices of the Royal Astronomical Society, 2020, 498 (4), pp.5251-5262. ⟨10.1093/mnras/staa2571⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 498 (4), pp.5251-5262. ⟨10.1093/mnras/staa2571⟩
We present 2000 mock galaxy catalogues for the analysis of baryon acoustic oscillations (BAOs) in the Emission Line Galaxy (ELG) sample of the extended Baryon Oscillation Spectroscopic Survey Data Release 16 (eBOSS DR16). Each mock catalogue has a nu
Autor:
Anatoly Klypin, David E. Millán-Calero, Francisco Prada, Darren J. Croton, Bruno Altieri, Cristian A. Vega-Martínez, Taira Oogi, Sofía A. Cora, Manodeep Sinha, Sylvain de la Torre, Eric Jullo, José Ruedas, R. Benton Metcalf, Tomoaki Ishiyama
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 506 (3), pp.4210-4231. ⟨10.1093/mnras/stab1755⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 506 (3), pp.4210-4231. ⟨10.1093/mnras/stab1755⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 2021, 506 (3), pp.4210-4231. ⟨10.1093/mnras/stab1755⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 506 (3), pp.4210-4231. ⟨10.1093/mnras/stab1755⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
We introduce the Uchuu suite of large high-resolution cosmological N-body simulations. The largest simulation, named Uchuu, consists of 2.1 trillion (12 8003) dark matter particles in a box of side-length 2.0 h-1, Gpc$, with particle mass of 3.27 ×
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b90914e298262960a5582aa4ef8d5112
http://hdl.handle.net/10261/264963
http://hdl.handle.net/10261/264963
Autor:
Anatoly Klypin, Vladimir Avila-Reese, Aldo Rodríguez-Puebla, Vivian Poulin, Francisco Prada, Peter Behroozi, Joel R. Primack, Doug Hellinger, Marc Kamionkowski, Tristan L. Smith
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 504 (1), pp.769-781. ⟨10.1093/mnras/stab769⟩
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
instname
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 504 (1), pp.769-781. ⟨10.1093/mnras/stab769⟩
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Cold Dark Matter with cosmological constant (ΛCDM) cosmological models with early dark energy (EDE) have been proposed to resolve tensions between the Hubble constant H 0=100, h km -1pc-1 measured locally, giving h ≈ 0.73, and H0 deduced from Plan
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9af6bbce61c561843e1ccb8a3a880aca
http://hdl.handle.net/10261/248037
http://hdl.handle.net/10261/248037
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
Autor:
César Hernández-Aguayo, Cheng-Zong Ruan, Baojiu Li, Christian Arnold, Carlton M. Baugh, Anatoly Klypin, Francisco Prada
Publikováno v:
Journal of Cosmology and Astroparticle Physics, 2022, Vol.2022, pp.048 [Peer Reviewed Journal]
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the origina
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Making cosmological inferences from the observed galaxy clustering requires accurate predictions for the mean clustering statistics and their covariances. Those are affected by cosmic variance - the statistical noise due to the finite number of harmo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::518c96eeedc100981cf20c8dd739dfcc
http://hdl.handle.net/10261/221585
http://hdl.handle.net/10261/221585
Autor:
Ghassem Gozaliasl, Esra Bulbul, Charles C. Fitzpatrick, Florian Pacaud, Francisco Prada, Erwin T. Lau, Daisuke Nagai, Dominique Eckert, Chia-Hsun Chiang, Nicolas Clerc, Gustavo Yepes, Jeremy S. Sanders, Violeta Gonzalez-Perez, Johan Comparat, Vittorio Ghirardini, Thomas H. Reiprich, Anatoly Klypin, Alexis Finoguenov, Marra Salvato, Jacob Ider Chitham, Kirpal Nandra, Elmo Tempel, Miriam E. Ramos-Ceja, Florian Kfer, Andrea Merloni, R. Seppi, R. W. Schmidt, Teng Liu
Publikováno v:
Open J.Astrophys.
Open J.Astrophys., 2020, 3, pp.13. ⟨10.21105/astro.2008.08404⟩
Open J.Astrophys., 2020, 3, pp.13. ⟨10.21105/astro.2008.08404⟩
The eROSITA X-ray telescope on board the Spectrum-Roentgen-Gamma (SRG) mission will measure the position and properties of about 100,000 clusters of galaxies and 3 million active galactic nuclei over the full sky. To study the statistical properties
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ba91845abc832c6b2e52aaa3e43ef5b8
https://hal.archives-ouvertes.fr/hal-02939983
https://hal.archives-ouvertes.fr/hal-02939983