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Record W6930753306 · doi:10.5281/zenodo.15814299

Systematic Identification of g-Mode Pulsations in Subdwarf B Stars for Kepler Data

2025· article· en· W6930753306 on OpenAlexaboutno aff

Bibliographic record

VenueZenodo (CERN European Organization for Nuclear Research) · 2025
Typearticle
Languageen
FieldSocial Sciences
TopicVaccine Coverage and Hesitancy
Canadian institutionsnot available
Fundersnot available
KeywordsAsteroseismologySpectral lineStarsSubdwarfRotation periodMode (computer interface)Parameter spaceStellar classification

Abstract

fetched live from OpenAlex

The Kepler and TESS space missions have revealed the g-mode pulsation spectra of many sdB stars, showing complex behaviors, with some stars exhibiting trapped modes interposed in the asymptotic period sequences of regular period spacing, while others do not. We used the STELUM (STELlar modeling at the Université de Montréal) to compute static and evolutionary models of sdB stars with different prescriptions for their chemical and thermal structures, and our PULSE code to compute their associated theoretical spectra from degrees l=1 to l=4 and for periods between 1000s and 15000s, thus covering the range of observed g-modes in such stars. Our results show that the structure of g- modes spectra, and notably the appearance of trapped modes, are dependent on the chemical and thermal structures of the models, and in particular on the region above the He-burning core. We mainly observe three flavors of spectra for mid to high radial orders g-modes: ”flat” spectra of nearly constant period spacing, spectra with regular mode trapping, and spectra of ”wavy” patterns in period spacing. In the two later types of spectra, we identified the region where modes are trapped in the star. The next natural step is comparing observed g-mode spectra to our theoretical models to constrain by asteroseismology the internal structure of sdB stars, and in particular the region above the He-burning core. This starts by extracting and analyzing the g-modes frequencies from available observations, which reach hundreds of frequencies in Kepler datasets, including rotational multiplets and frequency modulation effects. Given this large number of frequencies, and rotational multiplets generally being present for only a minority of them, identifying the degree of each frequency, and thus the pulsation spectra associated to a star, is complex and often includes an arbitrary component, especially in the case of stars presenting mode trapping. We thus aim at making mode identification a systematic process for slow rotating sdB pulsators, through a genetic algorithm currently in development. The latter takes advantages of continuous sequences of l=1 and l=2 modes found in Kepler data for sdB stars, overlapping properties between degrees, and offsets in periods induced by mode trapping, to infer the most likely degree for a given frequency.

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)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.004

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0030.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.061
GPT teacher head0.340
Teacher spread0.279 · 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 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

Citations0
Published2025
Admission routes1
Has abstractyes

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