The Three Hundred project: A large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications

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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 properties and scaling relations.We find that the modelle...

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Autor principal: Cui, W.
Otros Autores: Knebe, A., Yepes, G., Pearce, F., Power, C., Dave, R., Arth, A., Borgani, S., Dolag, K., Elahi, P., Mostoghiu, R., Murante, G., Rasia, E., Stoppacher, D., Vega-Ferrero, J., Wang, Y., Yang, X., Benson, A., Cora, S.A, Croton, D.J, Sinha, M., Stevens, A.R, Vega-Martínez, C.A, Arthur, J., Baldi, A.S, Cañas, R., Cialone, G., Cunnama, D., Marco, P.D, Durando, G., Ettori, S., Gottlöber, S., Nuza, S.E, Old, L.J, Pilipenko, S., Sorce, J.G, Welker, C.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: Oxford University Press 2018
Acceso en línea:Registro en Scopus
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Biblioteca Central Dr. Luis F. Leloir (FCEN) de Universidad de Buenos Aires
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030 |a MNRAA 
100 1 |a Cui, W. 
245 1 4 |a The Three Hundred project: A large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications 
260 |b Oxford University Press  |c 2018 
506 |2 openaire  |e Política editorial 
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520 3 |a 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 properties and scaling relations.We find that the modelled galaxy clusters are generally in reasonable agreement with observations with respect to baryonic fractions and gas scaling relations at redshift z = 0. However, there are still some (model-dependent) differences, such as central galaxies being too massive, and galaxy colours (g - r) being bluer (about 0.2 dex lower at the peak position) than in observations. The agreement in gas scaling relations down to 10 13 h -1 M· between the simulations indicates that particulars of the sub-grid modelling of the baryonic physics only has a weak influence on these relations.We also include - where appropriate - a comparison to three semi-analytical galaxy formation models as applied to the same underlying dark-matteronly simulation. All simulations and derived data products are publicly available. © 2018 The Author(s).  |l eng 
536 |a Detalles de la financiación: Ministerio de Economía y Competitividad, MINECO 
536 |a Detalles de la financiación: National Natural Science Foundation of China, NSFC, 11233005 
536 |a Detalles de la financiación: National Natural Science Foundation of China, NSFC, 11621303 
536 |a Detalles de la financiación: The work has received financial support from the European Union's Horizon 2020 Research and Innovation programme under the Marie Sklodowskaw-Curie grant agreement number 734374, i.e. the LACEGAL project.14 The workshop where this work has been finished was sponsored in part by the Higgs Centre for Theoretical Physics at the University of Edinburgh. The authors would like to thank The Red Española de Supercomputaci ón for granting us computing time at the MareNostrum Supercomputer of the BSC-CNS where most of the cluster simulations have been performed. The MDPL2 simulation has been performed at LRZ Munich within the project pr87yi. The CosmoSim database (https://www.cosmosim.org) is a service by the Leibniz Institute for Astrophysics Potsdam (AIP). Part of the computations with GADGETX have also been performed at the 'Leibniz-Rechenzentrum' with CPU time assigned to the Project 'pr83li'. This work has made extensive use of the PYTHON packages-IPYTHON with its Jupyter notebook (Pérez & Granger 2007), NUMPY (van der Walt, Colbert & Varoquaux 2011), and SCIPY (Oliphant 2007; Millman & Aivazis 2011). All the figures in this paper are plotted using the python MATPLOTLIB package (Hunter 2007). This research has made use of NASA's Astrophysics Data System and the arXiv preprint server. WC, AK, GY, and RM are supported by the Ministerio de Economía y Competitividad and the Fondo Europeo de Desarrollo Regional (MINECO/FEDER, UE) in Spain through grant AYA2015-63810-P. WC further thanks TaiLai Cui for all the joys. AK is also supported by the Spanish Red Consolider MultiDark FPA2017-90566-REDC and further thanks Krog for making the days counts. CP acknowledges the Australia Research Council (ARC) Centre of Excellence (CoE) ASTRO 3D through project number CE170100013. PJE is supported by the ARC CoE ASTRO 3D through project number CE170100013. SB acknowledged financial support from PRIN-MIUR grant 2015W7KAWC, the agreement ASI-INAF n.2017-14-H.0, the INFN INDARK grant, the EU H2020 Research and Innovation Programme under the ExaNeSt project (Grant Agreement No. 671553). ER acknowledges the ExaNeSt and Euro Exa projects, funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No. 671553 and No. 754337 and financial contribution from the agreement ASI-INAF n.2017-14-H.0. DS' fellowship is funded by the Spanish Ministry of Economy and Competitiveness (MINECO) under the 2014 Severo Ochoa Predoctoral Training Programme. J.V-F acknowledges the hospitality of the Physics & Astronomy Department at the University of Pennsylvania for hosting him during the preparation of this work. YW is supported by the national science foundation of China (No. 11643005). XY is supported by the National Key Basic Research Program of China (No. 2015CB857002), national science foundation of China (No. 11233005, 11621303). JTA acknowledges support from a postgraduate award from STFC. SAC acknowledges funding from Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET, PIP-0387), Agencia Nacional de Promoción Científica y Tecnol ógica (ANPCyT, PICT-2013-0317), and Universidad Nacional de La Plata(G11-124), Argentina. CVM acknowledges CONICET, Argentina, for their supporting fellowships. ASB, GC, and MDP are supported by Sapienza University of Rome-Progetti di Ricerca Anno 2016. ASB also acknowledges funding from Sapienza Uni-14https://cordis.europa.eu/project/rcn/207630 en.html versità di Roma under minor grant Progetti per Avvio alla Ricerca Anno 2017, prot. AR11715C82402BC7. RC is supported by the MERAC foundation postdoctoral grant awarded to Claudia Lagos and by the Consejo Nacional de Ciencia y Tecnología CONACYT CVU 520137 Scholar 290609 Overseas Scholarship 438594. SE acknowledges financial contribution from the contracts NARO15 ASI-INAF I/037/12/0, ASI 2015-046-R.0, and ASI-INAF n.2017-14-H.0. SEN is a member of the Carrera del Investigador Científico of CONICET. SP is supported by the Fundamental Research Program of Presidium of the RAS #28. JS acknowledges support from the "Centre National d'études spatiales" (CNES) postdoctoral fellowship program as well as from the "l'Oréal-UNESCO pour les femmes et la Science" fellowship program 
593 |a Departamento de Física Teórica, Módulo 15 Universidad Autónoma de Madrid, Madrid, E-28049, Spain 
593 |a Centro de Investigacion Avanzada en Física Fundamental (CIAFF), Universidad Autónoma de Madrid, Madrid, E-28049, Spain 
593 |a International Centre for Radio Astronomy Research, The University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia 
593 |a School of Physics and Astronomy, University of Nottingham, Nottingham, NG7 2RD, United Kingdom 
593 |a Institute for Astronomy, School of Physics and Astronomy, The University of Edinburgh, Royal Observatory, Edinburgh, EH9 3HJ, United Kingdom 
593 |a University Observatory Munich, Scheinerstraße 1, Munich, D-81679, Germany 
593 |a Max-Planck-Institute for Extraterrestrial Physics, Giessenbachstrasse 1, Garching, D-85748, Germany 
593 |a Dipartimento di Fisica, Sezione di Astronomia, Universitá di Trieste, Via Tiepolo 11, Trieste, I-34143, Italy 
593 |a INAF - Osservatorio Astronomico di Trieste, Via Tiepolo 11, Trieste, I-34143, Italy 
593 |a INFN - Sezione di Trieste, Via Valerio 2, Trieste, I-34127, Italy 
593 |a Max-Planck Institute for Astrophysics, Karl-Schwarzschild-Strabetae 1, Garching, D-85741, Germany 
593 |a Instituto de Física Teórica, (UAM/CSIC), Universidad Autónoma de Madrid, Cantoblanco, Madrid, E-28049, Spain 
593 |a IFCA, Instituto de Física de Cantabria (UC-CSIC), Av. de Los Castros s/n, Santander, E-39005, Spain 
593 |a School of Physics and Astronomy, Sun Yat-sen University, Zhuhai, 519082, China 
593 |a Department of Astronomy, Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University, Shanghai, 200240, China 
593 |a IFSA Collaborative Innovation Center and Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai, 200240, China 
593 |a Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101, United States 
593 |a Instituto de Astrofísica de La Plata (CCT La Plata CONICET, UNLP), Paseo del Bosque s/n, La Plata, B1900FWA, Argentina 
593 |a Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque s/n, La Plata, B1900FWA, Argentina 
593 |a Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia 
593 |a Department of Physics, Sapienza Università di Roma, P.le Aldo Moro 5, Rome, I-00185, Italy 
593 |a Dipartimento di Fisica, Università di Roma Tor Vergata, Via della Ricerca Scientifica 1, Roma, I-00133, Italy 
593 |a South African Astronomical Observatory, PO Box 9, Observatory, Cape Town, 7935, South Africa 
593 |a Department of Physics and Astronomy, University of the Western Cape, Cape Town, 7535, South Africa 
593 |a INFN - Sezione di Roma, P.le A. Moro 2, Roma, I-00185, Italy 
593 |a Dipartimento diFisica, Università degli Studi di Torino, ViaPietroGiuria, 1, Torino, I-10125, Italy 
593 |a INAF,Osservatorio di Astrofisica e Scienza dello Spazio, Via PietroGobetti 93/3, Bologna, I-40129, Italy 
593 |a INFN, Sezione di Bologna, Viale Berti Pichat 6/2, Bologna, I-40127, Italy 
593 |a Leibniz-Institut für Astrophysik, Potsdam, D-14482, Germany 
593 |a Instituto de Astronomía y Física del Espacio (IAFE CONICET-UBA), CC 67, Suc. 28, Buenos Aires, 1428, Argentina 
593 |a Facultad de Ciencias Exactas y Naturales (FCEyN), Universidad de Buenos Aires (UBA), Buenos Aires, 1053, Argentina 
593 |a Department of Astronomy and Astrophysics, University of Toronto, Toronto, Canada 
593 |a Astro Space Centre of Lebedev Physical Institute, Russian Academy of Sciences, Profsoyuznaja 84/32, Moscow, 117997, Russian Federation 
593 |a Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon, UMR5574, Saint-Genis-Laval, F-69230, France 
593 |a CNRS and UPMC Univ. Paris 06, UMR 7095, Institut d'Astrophysique de Paris, 98 bis Boulevard Arago, Paris, F-75014, France 
690 1 0 |a GALAXIES: CLUSTERS: GENERAL 
690 1 0 |a GALAXIES: CLUSTERS: INTRACLUSTER MEDIUM 
690 1 0 |a GALAXIES: GENERAL 
690 1 0 |a GALAXIES: HALOES 
700 1 |a Knebe, A. 
700 1 |a Yepes, G. 
700 1 |a Pearce, F. 
700 1 |a Power, C. 
700 1 |a Dave, R. 
700 1 |a Arth, A. 
700 1 |a Borgani, S. 
700 1 |a Dolag, K. 
700 1 |a Elahi, P. 
700 1 |a Mostoghiu, R. 
700 1 |a Murante, G. 
700 1 |a Rasia, E. 
700 1 |a Stoppacher, D. 
700 1 |a Vega-Ferrero, J. 
700 1 |a Wang, Y. 
700 1 |a Yang, X. 
700 1 |a Benson, A. 
700 1 |a Cora, S.A. 
700 1 |a Croton, D.J. 
700 1 |a Sinha, M. 
700 1 |a Stevens, A.R. 
700 1 |a Vega-Martínez, C.A. 
700 1 |a Arthur, J. 
700 1 |a Baldi, A.S. 
700 1 |a Cañas, R. 
700 1 |a Cialone, G. 
700 1 |a Cunnama, D. 
700 1 |a Marco, P.D. 
700 1 |a Durando, G. 
700 1 |a Ettori, S. 
700 1 |a Gottlöber, S. 
700 1 |a Nuza, S.E. 
700 1 |a Old, L.J. 
700 1 |a Pilipenko, S. 
700 1 |a Sorce, J.G. 
700 1 |a Welker, C. 
773 0 |d Oxford University Press, 2018  |g v. 480  |h pp. 2898-2915  |k n. 3  |p Mon. Not. R. Astron. Soc.  |x 00358711  |w (AR-BaUEN)CENRE-6169  |t Monthly Notices of the Royal Astronomical Society 
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856 4 0 |u https://doi.org/10.1093/mnras/sty2111  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_00358711_v480_n3_p2898_Cui  |y Handle 
856 4 0 |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v480_n3_p2898_Cui  |y Registro en la Biblioteca Digital 
961 |a paper_00358711_v480_n3_p2898_Cui  |b paper  |c PE 
962 |a info:eu-repo/semantics/article  |a info:ar-repo/semantics/artículo  |b info:eu-repo/semantics/publishedVersion 
999 |c 86089 

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