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Record W4408537894 · doi:10.1051/0004-6361/202453508

TOI-6508 b: A massive transiting brown dwarf orbiting a low-mass star

2025· article· en· W4408537894 on OpenAlexaff
K. Barkaoui, Daniel Sebastian, Sebastián Zúñiga-Fernández, A. H. M. J. Triaud, Benjamin V. Rackham, Adam J. Burgasser, T.W. Carmichael, M. Gillon, Christopher A. Theissen, Emma Softich, B. Rojas-Ayala, G. Srdoc, A. Soubkiou, A. Fukui, M. Timmermans, M. Stalport, A. Burdanov, D.R. Ciardi, K.A. Collins, Yasmin Davis, Fatemeh Davoudi, J. de Wit, B. -O. Demory, Sarah Deveny, G. Dransfield, Elsa Ducrot, L. Florian, Tianjun Gan, Y. Gómez Maqueo Chew, M. J. Hooton, S. B. Howell, J.M. Jenkins, Colin Littlefield, F. Murgas, Prajwal Niraula, E. Palle, P.P. Pedersen, F. J. Pozuelos, D. Queloz, G. Ricker, R.P. Schwarz, S. Seager, A. Shporer, M. G. Scott, C. Stockdale, Joshua N. Winn

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversité de Montréal
FundersAgencia Estatal de InvestigaciónScience and Technology Facilities CouncilScience Mission DirectorateAgencia Nacional de Investigación y DesarrolloMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesMinisterio de Ciencia e InnovaciónNuclear Safety and Security CommissionFonds De La Recherche Scientifique - FNRSCalifornia Institute of TechnologyEuropean CommissionMinistry of Science, ICT and Future PlanningAmes Research CenterFédération Wallonie-BruxellesKorea Astronomy and Space Science InstituteNational Aeronautics and Space AdministrationFonds pour la Formation à la Recherche dans l’Industrie et dans l’AgricultureEuropean Southern ObservatorySpace Telescope Science InstituteNational Science Foundation
KeywordsPhysicsAstrophysicsBrown dwarfAstronomyStar (game theory)Circumbinary planetStars

Abstract

fetched live from OpenAlex

We report the discovery of a transiting brown dwarf orbiting a low-mass star, TOI-6508 b. Today, only ∼50 transiting brown dwarfs have been discovered. TOI-6508 b was first detected with data from the Transiting Exoplanet Survey Satellite (TESS) in Sectors 10, 37 and 63. Ground-based follow-up photometric data were collected with the SPECULOOS-South (Search for habitable Planets EClipsing ULtra-cOOl Stars) and LCOGT-1m telescopes, and RV measurements were obtained with the Near InfraRed Planet Searcher (NIRPS) spectrograph. We find that TOI-6508 b has a mass of Mp = 72.5−5.1+7.6 MJup and a radius of Rp = 1.03 ± 0.03 RJup. Our modeling shows that the data are consistent with an eccentric orbit of 19 day and an eccentricity of e = 0.28−0.08+0.09. TOI-6508 b has a mass ratio of MBD/M★ = 0.40, makes it the second highest mass ratio brown dwarf that transits a low-mass star. The host has a mass of M★ = 0.174 ± 0.004 M⊙, a radius of R★ = 0.205 ± 0.006 R⊙, an effective temperature of Teff = 2930 ± 70 K, and a metallicity of [Fe/H] = −0.22 ± 0.08. This makes TOI-6508 b an interesting discovery that has come to light in a region still sparsely populated.

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)0.000
metaresearch head score (Gemma)0.000
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 score0.006

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0010.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.006
GPT teacher head0.202
Teacher spread0.196 · 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

Citations13
Published2025
Admission routes1
Has abstractyes

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