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Record W4409048314 · doi:10.1051/0004-6361/202554064

The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations

2025· article· en· W4409048314 on OpenAlexfundno aff
Jonathan S. Gómez, Tomás Hough, A. Jiménez Muñoz, Gustavo Yepes, Weiguang Cui, S. A. Cora

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstronomy and Astrophysical Research
Canadian institutionsnot available
FundersAgencia Estatal de InvestigaciónBarcelona Supercomputing CenterMinisterio de Ciencia e InnovaciónUniversidad Autónoma de MadridScience and Technology Facilities CouncilUniversity of TorontoConsejo Nacional de Investigaciones Científicas y TécnicasUniversidad Nacional de La PlataUniversity of LeicesterAlliance de recherche numérique du CanadaComunidad de MadridUK Research and InnovationInnovation, Science and Economic Development Canada
KeywordsPhysicsAstrophysicsCluster (spacecraft)GalaxyGalaxy clusterBrightest cluster galaxyType-cD galaxyGalaxy formation and evolutionAstronomy

Abstract

fetched live from OpenAlex

Next-generation photometric and spectroscopic surveys will detect faint galaxies in massive clusters, advancing our understanding of galaxy formation in dense environments. Comparing these observations with theoretical models requires high-resolution cluster simulations. Hydrodynamical simulations effectively resolve galaxy properties in halos; however, they face challenges in simulating low-mass galaxies within massive clusters due to computational limitations. On the other hand, dark matter-only (DMO) simulations can provide higher resolution but need models to populate subhalos with galaxies. In this work, we introduce a fast and efficient emulator of hydrodynamical simulations of galaxy clusters, based on the semi-analytic models (SAMs) SAGE and SAG. The calibration of the cluster galaxy properties in the SAMs was guided by the cluster galaxies from the hydrodynamical simulations at intermediate resolution, which represents the highest resolution achievable with current hydrodynamical simulations, ensuring consistency in properties such as stellar masses and luminosities across different redshifts. These SAMs are then applied to DMO simulations from THE THREE HUNDRED Project at three different resolutions. Our results show that the SAG model, unlike SAGE, more efficiently emulates the galaxy properties tested in this study even at the highest resolution. This improvement results from the detailed treatment of orphan galaxies, which are satellite galaxies that contribute significantly to the overall galaxy population. SAG enables the study of dwarf galaxies down to stellar masses of M* = 107 M⊙ at the highest resolution, which is an order of magnitude smaller than the stellar masses of galaxies in the hydrodynamical simulations at the intermediate resolution, corresponding to approximately four magnitudes fainter. This demonstrates that a SAM can be effectively calibrated to provide fast and accurate predictions for specific hydrodynamical simulations, offering a computationally efficient alternative for exploring galaxy populations in dense environments across higher resolutions.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.004
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Methods · Consensus signal: Methods
Teacher disagreement score0.007
Threshold uncertainty score0.018

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.004
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0000.001
Science and technology studies0.0000.001
Scholarly communication0.0010.001
Open science0.0030.001
Research integrity0.0010.002
Insufficient payload (model declined to judge)0.0050.001

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 head0.011
GPT teacher head0.275
Teacher spread0.264 · 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 source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreMethods

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

Citations0
Published2025
Admission routes1
Has abstractyes

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