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Record W4409449783 · doi:10.1051/0004-6361/202452659

Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations

2025· article· en· W4409449783 on OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

fundA Canadian funder is recorded on the work.
no affNo Canadian affiliation: this work is invisible to an affiliation-only frame.
No Canadian affiliation. An affiliation-only frame, the usual design, would never have seen this work. It is one of the works that make the case for inverting the frame.

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldMathematics
TopicModeling, Simulation, and Optimization
Canadian institutionsnot available
FundersNederlandse Organisatie voor Wetenschappelijk OnderzoekUniversity of TorontoRijksuniversiteit Groningen
KeywordsPhysicsAstrophysics

Abstract

fetched live from OpenAlex

Aims. Hierarchical merging of galaxies plays an important role in galaxy formation and evolution. Mergers could trigger key evolutionary phases such as starburst activities and active accretion periods onto supermassive black holes at the centres of galaxies. We aim to detect mergers and merger stages (pre- and post-mergers) across cosmic history. Our main goal is to test whether it is more beneficial to detect mergers and their merger stages simultaneously or hierarchically. In addition, we wish to test the impact of merger time relative to the coalescence of merging galaxies. Methods. First, we generated realistic mock James Webb Space Telescope (JWST) images of simulated galaxies selected from the IllustrisTNG cosmological hydrodynamical simulations. The advantage of using simulations is that we have information on both whether a galaxy is a merger and its exact merger stage (i.e. when in the past or in the future the galaxy has experienced or will experience a merging event). Then, we trained deep-learning (DL) models for galaxy morphology classifications in the Zoobot Python package to classify galaxies into non-merging galaxies, merging galaxies and their merger stages. We used two different set-ups, a two-stage set-up versus a one-stage set-up. In the former set-up, we first classified galaxies into mergers and non-mergers, and we then classified the mergers into pre-mergers and post-mergers. In the latter set-up, non-mergers, pre-mergers and post-mergers were classified simultaneously. Results. We found that the one-stage classification set-up moderately outperforms the two-stage set-up. It offers a better overall accuracy and generally a better precision, particularly for the non-merger class. Out of the three classes, pre-mergers can be classified with the highest precision (∼65% versus ∼33% from a random classifier) in both set-ups, possibly because the merging features are generally more easily recognised, and because there are merging companions. More confusion is found between post-mergers and non-mergers than between these two classes and pre-mergers. The image signal-to-noise ratio (S/N) also affects the performance of the DL classifiers, but not by much after a certain threshold is crossed (S/N ∼ 20 in a 0.2″aperture). In terms of the merger timescale, both precision and recall of the classifiers strongly depend on merger time. Both set-ups find it more difficult to identify true mergers that are observed at stages that are farther from coalescence either in the past or in the future. For pre-mergers, we recommend selecting mergers that will merge in the next 0.4 Gyr to achieve a good balance between precision and recall.

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.

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: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.358
Threshold uncertainty score0.496

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 studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
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 head0.017
GPT teacher head0.266
Teacher spread0.249 · 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