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Record W2887742289 · doi:10.1093/mnras/sty2111

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

2018· article· en· W2887742289 on OpenAlexaff
Weiguang Cui, Alexander Knebe, Gustavo Yepes, F. R. Pearce, Chris Power, Romeel Davé, Alexander Arth, S. Borgani, Klaus Dolag, Pascal J. Elahi, Robert Mostoghiu, Giuseppe Murante, Elena Rasia, Doris Stoppacher, Jesús Vega-Ferrero, Yang Wang, Xiaohu Yang, Andrew Benson, S. A. Cora, Darren Croton, Manodeep Sinha, Adam R. H. Stevens, Cristian A Vega-Martínez, Jake Arthur, A. Baldi, Rodrigo Cañas, Giammarco Cialone, Daniel Cunnama, M. De Petris, Giacomo Durando, S. Ettori, Stefan Gottlöber, Sebastián E. Nuza, Lyndsay Old, Sergey Pilipenko, Jenny G. Sorce, Charlotte Welker

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of Toronto
FundersLeibniz-RechenzentrumInstituto Nazionale di Fisica NucleareLeibniz-GemeinschaftAustralian Research CouncilHorizon 2020 Framework ProgrammeSapienza Università di RomaScience and Technology Facilities CouncilMinistero dell’Istruzione, dell’Università e della RicercaConsejo Nacional de Investigaciones Científicas y TécnicasUniversidad Nacional de La PlataMinisterio de Economía y CompetitividadNational Natural Science Foundation of ChinaEuropean Regional Development FundEuropean CommissionUniversity of EdinburghLeibniz-Institut für Astrophysik PotsdamUniversity of PennsylvaniaNational Aeronautics and Space AdministrationAgencia Nacional de Promoción Científica y TecnológicaConsejo Nacional de Ciencia y TecnologíaFondation MeracNational Science Foundation
KeywordsPhysicsAstrophysicsRedshiftGalaxyGalaxy clusterGalaxy formation and evolutionScalingBaryonDark matterCluster (spacecraft)

Abstract

fetched live from OpenAlex

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 dataset 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 semianalytical galaxy formation models as applied to the same underlying dark matter only simulation. All simulations and derived data products are publicly available.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.482
Threshold uncertainty score0.514

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.001
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.008
GPT teacher head0.213
Teacher spread0.205 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations229
Published2018
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicGalaxies: Formation, Evolution, PhenomenaFrench-language works237,207