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

dc.contributor.authorCui, Weiguang
dc.contributor.authorKnebe, Alexander 
dc.contributor.authorYepes Alonso, Gustavo 
dc.contributor.authorPearce, Frazer R.
dc.contributor.authorPower, Chris
dc.contributor.authorDave, Romeel
dc.contributor.authorArth, Alexander
dc.contributor.authorBorgani, Stefano
dc.contributor.authorDolag, Klaus
dc.contributor.authorElahi, Pascal
dc.contributor.authorMostoghiu, Robert
dc.contributor.authorMurante, Giuseppe
dc.contributor.authorRasia, Elena
dc.contributor.authorStoppacher , Doris 
dc.contributor.authorVega Ferrero, Jesús
dc.contributor.authorWang, Yang 
dc.contributor.authorYang, Xiaohu
dc.contributor.authorBenson, Andrew
dc.contributor.authorCora, Sofía A.
dc.contributor.authorCroton, Darren J.
dc.contributor.authorSinha, Manodeep
dc.contributor.authorStevens, Adam R.H.
dc.contributor.authorVega-Martínez, Cristian A.
dc.contributor.authorArthur, Jake
dc.contributor.authorBaldi, Anna S.
dc.contributor.authorCañas, Rodrigo
dc.contributor.authorCialone, Giammarco
dc.contributor.authorCunnama, Daniel
dc.contributor.authorMarco, De Petris
dc.contributor.authorDurando, Giacomo
dc.contributor.authorEttori, Stefano
dc.contributor.authorGottlöber, Stefan
dc.contributor.authorNuza, Sebastián E.
dc.contributor.authorOld, Lyndsay J.
dc.contributor.authorPilipenko, Sergey
dc.contributor.authorSorce, Jenny G.
dc.contributor.authorWelker, Charlotte
dc.contributor.otherUAM. Departamento de Física Teóricaes_ES
dc.contributor.otherUAM. Centro de Investigación Avanzada en Física Fundamental (CIAFF-UAM)es_ES
dc.date.accessioned2019-02-26T14:05:05Z
dc.date.available2019-02-26T14:05:05Z
dc.date.issued2018-08-03
dc.identifier.citationMonthly Notices of the Royal Astronomical Society 480.3 (2018): 2898-2915en_US
dc.identifier.issn0035-8711 (print)es_ES
dc.identifier.issn1365-2966 (online)es_ES
dc.identifier.urihttp://hdl.handle.net/10486/686737
dc.description.abstractWe 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 1013 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-matter only simulation. All simulations and derived data products are publicly available.en_US
dc.description.sponsorshipThe 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 project14. The workshop where this work has been finished was sponsored in part by the Higgs Centre for Theoretical Physics at the University of Edinburgh´ 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 (崔泰莱) 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 acknowledge 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 Tecnológica (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 Universit_a 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 fi- nancial 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 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'etudes spatiales" (CNES) postdoctoral fellowship program as well as from the “l'Oreal-UNESCO pour les femmes et la Science" fellowship programen_US
dc.format.extent21 pag.es_ES
dc.format.mimetypeapplication/pdfen
dc.language.isoengen
dc.publisherOxford University Press on behalf of the Royal Astronomical Societyen_US
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen_US
dc.rights© 2018 The Author(s)es_ES
dc.subject.otherGalaxies: clusters: generalen_US
dc.subject.otherGalaxies: clusters: intracluster mediumen_US
dc.subject.otherGalaxies: generalen_US
dc.subject.otherGalaxies: haloesen_US
dc.titleThe Three Hundred project: A large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applicationsen_US
dc.typepreprinten
dc.subject.ecienciaFísicaes_ES
dc.relation.publisherversionhttps://doi.org/10.1093/mnras/sty2111es_ES
dc.identifier.doi10.1093/mnras/sty2111es_ES
dc.identifier.publicationfirstpage2898es_ES
dc.identifier.publicationissue3es_ES
dc.identifier.publicationlastpage2915es_ES
dc.identifier.publicationvolume480es_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/H2020/734374/EU//MSCes_ES
dc.relation.projectIDGobierno de España. AYA2015-63810-Pes_ES
dc.type.versioninfo:eu-repo/semantics/submittedVersionen
dc.rights.accessRightsopenAccessen
dc.authorUAMKnebe , Alexander (262044)
dc.authorUAMYepes Alonso, Gustavo (260625)
dc.authorUAMVega Ferrero, Jesús (264865)
dc.facultadUAMFacultad de Ciencias


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