MétaCan
Menu
← Back to cohort
Record W4415719810 · doi:10.1093/mnras/staf1052

The <scp>thesan–zoom</scp> project: long-term imprints of external reionization on galaxy evolution

2025· article· en· W4415719810 on OpenAlexafffund
Oliver Zier, Rahul Kannan, Aaron Smith, Ewald Puchwein, Mark Vogelsberger, Josh Borrow, Enrico Garaldi, Laura C. Keating, William McClymont, Xuejian Shen, Lars Hernquist

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsYork University
FundersScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaNational Aeronautics and Space Administration
KeywordsReionizationGalaxyRedshiftMetallicityRadiative transferStar formationGalaxy formation and evolutionStars

Abstract

fetched live from OpenAlex

ABSTRACT We investigate the impact of ionizing external ultraviolet (UV) radiation on low-mass haloes ($M_\text{halo}\lesssim 10^{10}\, {\rm M_\odot }$) at high redshift ($z\ge 3$) using $1140\, {\rm M_\odot }$ baryonic resolution zoom-in simulations of seven thesan–zoom regions. We compare three simulation sets that differ in the treatment of external UV radiation: one employing a uniform UV background initiated at $z=10.6$ in addition to radiation transport for local sources, another with the background starting at $z=5.5$, and the default configuration using the large-scale radiation from the parent thesan-1 simulation as a boundary condition. The multiphase interstellar medium (ISM) model, combined with its high mass resolution, allows us to resolve all star-forming haloes and capture the back-reaction of ionizing radiation on galaxy properties during the epoch of reionization. When present, external UV radiation efficiently unbinds gas in haloes with masses below $10^9{\, \rm M_\odot }$ and suppresses subsequent star formation. As a result, in simulations with early reionization, minihaloes fail to form stars from pristine gas, leading to reduced metal enrichment of gas later accreted by more massive haloes. Consequently, haloes with masses below $10^{10}{\, \rm M_\odot }$ at all simulated epochs ($z>3$) exhibit lower metallicities and altered metallicity distributions. The more accurate and realistic shielding from external UV radiation, achieved through self-consistent radiative transfer, permits the existence of a cold but low-density gas phase down to $z=3$. These findings highlight the importance of capturing a patchy reionization in high-resolution simulations targeting high-redshift galaxy formation. We conclude that at minimum, semi-numerical models that incorporate spatially inhomogeneous reionization and a non-uniform metallicity floor are necessary to accurately emulate metal enrichment in minihaloes.

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)0.001
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: Empirical · Consensus signal: Empirical
Teacher disagreement score0.023
Threshold uncertainty score0.046

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0000.000
Science and technology studies0.0000.001
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0060.000

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 head0.006
GPT teacher head0.213
Teacher spread0.207 · 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
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

Citations4
Published2025
Admission routes2
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→