Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Cialone Giammarco"'
Autor:
De Petris Marco, Ruppin Florian, Sembolini Federico, Adam Remí, Baldi Anna Silvia, Cialone Giammarco, Comis Barbara, De Luca Federico, Gianfagna Giulia, Kéruzoré Florian, Macías-Pérez Juan, Mayet Frédéric, Perotto Laurence, Yepes Gustavo
Publikováno v:
EPJ Web of Conferences, Vol 228, p 00008 (2020)
The NIKA2 Sunyaev-Zel’dovich Large Program (SZLP) is focused on mapping the thermal SZ signal of a representative sample of selected Planck and ACT clusters spanning the redshift range 0.5 < z < 0.9. Hydrodynamical N-body simulations prove to be a
Externí odkaz:
https://doaj.org/article/37b0577b16374b019301157599410a1b
Autor:
Cui, Weiguang, Knebe, Alexander, Yepes, Gustavo, Pearce, Frazer, Power, Chris, Dave, Romeel, Arth, Alexander, Borgani, Stefano, Dolag, Klaus, Elahi, Pascal, Mostoghiu, Robert, Murante, Giuseppe, Rasia, Elena, Stoppacher, Doris, Vega-Ferrero, Jesus, Wang, Yang, Yang, Xiaohu, Benson, Andrew, Cora, Sofía A., Croton, Darren J., Sinha, Manodeep, Stevens, Adam R. H., Vega-Martínez, Cristian A., Arthur, Jake, Baldi, Anna S., Cañas, Rodrigo, Cialone, Giammarco, Cunnama, Daniel, De Petris, Marco, Durando, Giacomo, Ettori, Stefano, Gottlöber, Stefan, Nuza, Sebastián E., Old, Lyndsay J., Pilipenko, Sergey, Sorce, Jenny G., Welker, Charlotte
Publikováno v:
Cui, W., Knebe, A., Yepes, G., et al.\ 2018, \mnras, 480, 2898
We introduce the THE THREE HUNDRED project, an endeavour to model 324 large galaxy clusters with full-physics hydrodynamical re-simulations. Here we present the data set and study the differences to observations for fundamental galaxy cluster propert
Externí odkaz:
http://arxiv.org/abs/1809.04622
Autor:
Cialone, Giammarco, De Petris, Marco, Sembolini, Federico, Yepes, Gustavo, Baldi, Anna Silvia, Rasia, Elena
The determination of the morphology of galaxy clusters has important repercussion on their cosmological and astrophysical studies. In this paper we address the morphological characterisation of synthetic maps of the Sunyaev--Zel'dovich (SZ) effect pr
Externí odkaz:
http://arxiv.org/abs/1708.03325
Autor:
Hadji Hossein, Shariar, Acernese, Marco, Cardona, Tommaso, Cialone, Giammarco, Curianò, Federico, Mariani, Lorenzo, Marini, Veronica, Marzioli, Paolo, Parisi, Leonardo, Piergentili, Fabrizio, Santoni, Fabio
Publikováno v:
In The Journal of Space Safety Engineering March 2020 7(1):30-37
Autor:
Cialone, Giammarco, Gianfermo, Andrea, Di Cecco, Alessandra, Mari, Silvia, Cassisi, Santi, Santoni, Fabio, Piergentili, Fabrizio
Publikováno v:
In Advances in Space Research 1 January 2019 63(1):800-811
Autor:
Mayet, F., Catalano, A., Macías-Pérez, J.F., Perotto, L., De Petris, Marco, Ruppin, Florian, Sembolini, Federico, Adam, Remí, Baldi, Anna Silvia, Cialone, Giammarco, Comis, Barbara, De Luca, Federico, Gianfagna, Giulia, Kéruzoré, Florian, Macías-Pérez, Juan, Mayet, Frédéric, Perotto, Laurence, Yepes, Gustavo
Publikováno v:
EPJ Web of Conferences; 2020, Vol. 228, p1-6, 6p
Akademický článek
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Autor:
Stefano Ettori, Sebastián E. Nuza, Cristian A. Vega-Martínez, Darren J. Croton, Manodeep Sinha, Jake Arthur, Daniel Cunnama, Frazer R. Pearce, Doris Stoppacher, Yang Wang, Robert Mostoghiu, Weiguang Cui, Anna Silvia Baldi, Adam R. H. Stevens, Elena Rasia, Gustavo Yepes, Stefan Gottlöber, G. Murante, Rodrigo Cañas, S. V. Pilipenko, Sofía A. Cora, Jesus Vega-Ferrero, Jenny G. Sorce, Pascal J. Elahi, Alexander Knebe, Andrew J. Benson, Alexander Arth, Lyndsay Old, Stefano Borgani, Giacomo Durando, Marco De Petris, Giammarco Cialone, Charlotte Welker, Xiaohu Yang, Romeel Davé, Chris Power, Klaus Dolag
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Monthly Notices of the Royal Astronomical Society, 2018, 480, pp.2898-2915. ⟨10.1093/mnras/sty2111⟩
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Monthly Notices of the Royal Astronomical Society, 2018, 480, pp.2898-2915. ⟨10.1093/mnras/sty2111⟩
We introduce the THE THREE HUNDRED project, an endeavour to model 324 large galaxy clusters with full-physics hydrodynamical re-simulations. Here we present the data set and study the differences to observations for fundamental galaxy cluster propert
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a543fae4dc0b67acaa30e78b7500215
http://hdl.handle.net/20.500.12386/30012
http://hdl.handle.net/20.500.12386/30012