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Grant support

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.

Analysis of institutional authors

Cui, WeiguangCorresponding AuthorKnebe, AlexanderCorresponding AuthorYepes, GustavoCorresponding AuthorMostoghiu, RobertAuthorStoppacher, DorisAuthor

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November 26, 2018
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Article

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

Publicated to:MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 480 (3): 2898-2915 - 2018-08-01 480(3), DOI: 10.1093/mnras/sty2111

Authors: 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, Sofia A.; Croton, Darren J.; Sinha, Manodeep; Stevens, Adam R. H.; Vega-Martinez, Cristian A.; Arthur, Jake; Baldi, Anna S.; Canas, Rodrigo; Cialone, Giammarco; Cunnama, Daniel; De Petris, Marco; Durando, Giacomo; Ettori, Stefano; Gottlober, Stefan; Nuza, Sebastian E.; Old, Lyndsay J.; Pilipenko, Sergey; Sorce, Jenny G.; Welker, Charlotte;

Affiliations

Carnegie Observ, 813 Santa Barbara St, Pasadena, CA 91101 USA - Author
CNRS, F-75014 Paris, France - Author
INAF, Osservatorio Astrofis & Sci Spazio, Via Pietro Gobetti 93-3, I-40129 Bologna, Italy - Author
INAF, Osservatorio Astron Trieste, I-34143 Trieste, Italy - Author
INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy - Author
INFN, Sez Roma, Ple A Moro 2, I-00185 Rome, Italy - Author
INFN, Sez Trieste, I-34127 Trieste, Italy - Author
Leibniz Inst Astrophys, D-14482 Potsdam, Germany - Author
Max Planck Inst Astrophys, Karl Schwarzschild Strabetae 1, D-85741 Garching, Germany - Author
Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany - Author
Russian Acad Sci, Lebedev Phys Inst, Astro Space Ctr, Profsoyuznaja 84-32, Moscow 117997, Russia - Author
Sapienza Univ Roma, Dept Phys, Ple Aldo Moro 5, I-00185 Rome, Italy - Author
Shanghai Jiao Tong Univ, IFSA Collaborat Innovat Ctr, Shanghai 200240, Peoples R China - Author
Shanghai Jiao Tong Univ, Shanghai Key Lab Particle Phys & Cosmol, Dept Astron, Shanghai 200240, Peoples R China - Author
Shanghai Jiao Tong Univ, Tsung Dao Lee Inst, Shanghai 200240, Peoples R China - Author
South African Astron Observ, POB 9, ZA-7935 Cape Town, South Africa - Author
Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519082, Peoples R China - Author
Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia - Author
UAM, CSIC, Inst Fis Teor, E-28049 Madrid, Spain - Author
UBA, CONICET, IAFE, CC 67,Suc 28, RA-1428 Buenos Aires, DF, Argentina - Author
UBA, Fac Ciencias Exactas & Nat FCEyN, RA-1053 Buenos Aires, DF, Argentina - Author
UC, CSIC, Inst Fis Cantabria, IFCA, Av de Los Castros S-N, E-39005 Santander, Spain - Author
Univ Autonoma Madrid, CIAFF, E-28049 Madrid, Spain - Author
Univ Autonoma Madrid, Dept Fis Teor, Modulo 15, E-28049 Madrid, Spain - Author
Univ Edinburgh, Royal Observ, Sch Phys & Astron, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland - Author
Univ Lyon1, Univ Lyon, Ens Lyon, CNRS,Ctr Rech Astrophys Lyon,UMR5574, F-69230 St Genis Laval, France - Author
Univ Nacl La Plata, Fac Ciencias Astron & Geofis, Paseo Bosque S-N,B1900FWA, La Plata, Buenos Aires, Argentina - Author
Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England - Author
Univ Observ Munich, Scheinerstr 1, D-81679 Munich, Germany - Author
Univ Roma Tor Vergata, Dipartimento Fis, Via Ric Sci 1, I-00133 Rome, Italy - Author
Univ Torino, Dipartimento Fis, Via Pietro Giuria 1, I-10125 Turin, Italy - Author
Univ Toronto, Dept Astron & Astrophys, Toronto, ON, Canada - Author
Univ Trieste, Sez Astron, Dipartimento Fis, Via Tiepolo 11, I-34143 Trieste, Italy - Author
Univ Western Australia, Int Ctr Radio Astron Res, 35 Stirling Highway, Crawley, WA 6009, Australia - Author
Univ Western Cape, Dept Phys & Astron, ZA-7535 Bellville, South Africa - Author
UNLP, CONICET, CCT La Plata, Inst Astrofis La Plata, Paseo Bosque S-N,B1900FWA, La Plata, Buenos Aires, Argentina - Author
UPMC Univ Paris 06, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France - Author
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Abstract

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-circle dot 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.

Keywords

Dark-matter haloesGalactic nuclei feedbackGalaxies: clusters: generalGalaxies: clusters: intracluster mediumGalaxies: generalGalaxies: haloesHot gasInitial mass functionLuminosity functionParticle hydrodynamics simulationsRhapsody-g simulationsScaling relationsStar-formationX-ray-clusters

Quality index

Bibliometric impact. Analysis of the contribution and dissemination channel

The work has been published in the journal MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY due to its progression and the good impact it has achieved in recent years, according to the agency WoS (JCR), it has become a reference in its field. In the year of publication of the work, 2018, it was in position 15/69, thus managing to position itself as a Q1 (Primer Cuartil), in the category Astronomy & Astrophysics.

From a relative perspective, and based on the normalized impact indicator calculated from World Citations provided by WoS (ESI, Clarivate), it yields a value for the citation normalization relative to the expected citation rate of: 4.63. This indicates that, compared to works in the same discipline and in the same year of publication, it ranks as a work cited above average. (source consulted: ESI Nov 14, 2024)

This information is reinforced by other indicators of the same type, which, although dynamic over time and dependent on the set of average global citations at the time of their calculation, consistently position the work at some point among the top 50% most cited in its field:

  • Weighted Average of Normalized Impact by the Scopus agency: 5.47 (source consulted: FECYT Feb 2024)
  • Field Citation Ratio (FCR) from Dimensions: 75.24 (source consulted: Dimensions Jul 2025)

Specifically, and according to different indexing agencies, this work has accumulated citations as of 2025-07-09, the following number of citations:

  • WoS: 105
  • Scopus: 127
  • Google Scholar: 207

Impact and social visibility

From the perspective of influence or social adoption, and based on metrics associated with mentions and interactions provided by agencies specializing in calculating the so-called "Alternative or Social Metrics," we can highlight as of 2025-07-09:

  • The use, from an academic perspective evidenced by the Altmetric agency indicator referring to aggregations made by the personal bibliographic manager Mendeley, gives us a total of: 63.
  • The use of this contribution in bookmarks, code forks, additions to favorite lists for recurrent reading, as well as general views, indicates that someone is using the publication as a basis for their current work. This may be a notable indicator of future more formal and academic citations. This claim is supported by the result of the "Capture" indicator, which yields a total of: 63 (PlumX).

With a more dissemination-oriented intent and targeting more general audiences, we can observe other more global scores such as:

  • The Total Score from Altmetric: 7.25.
  • The number of mentions on the social network X (formerly Twitter): 1 (Altmetric).

It is essential to present evidence supporting full alignment with institutional principles and guidelines on Open Science and the Conservation and Dissemination of Intellectual Heritage. A clear example of this is:

  • The work has been submitted to a journal whose editorial policy allows open Open Access publication.
  • Assignment of a Handle/URN as an identifier within the deposit in the Institutional Repository: https://repositorio.uam.es/handle/10486/686737

Leadership analysis of institutional authors

This work has been carried out with international collaboration, specifically with researchers from: Argentina; Australia; Canada; China; France; Germany; Italy; Russia; South African Republic; United Kingdom; United States of America.

There is a significant leadership presence as some of the institution’s authors appear as the first or last signer, detailed as follows: First Author (CUI, WEIGUANG) .

the authors responsible for correspondence tasks have been CUI, WEIGUANG, KNEBE ., ALEXANDER and YEPES ALONSO, GUSTAVO.