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Record W4390837679 · doi:10.1051/0004-6361/202346999

TOI-4860 b, a short-period giant planet transiting an M3.5 dwarf

2024· article· en· W4390837679 on OpenAlexafffund
J. M. Almenara, X. Bonfıls, Edward M. Bryant, Andrés Jordán, G. Hébrard, Eder Martioli, A. C. M. Correia, N. Astudillo-Defru, Charles Cadieux, L. Arnold, Étienne Artigau, G. Á. Bakos, S. C. C. Barros, Daniel Bayliss, F. Bouchy, Gwenaël Boué, Rafael Brahm, A. Carmona, D. Charbonneau, David R. Ciardi, Ryan Cloutier, Marion Cointepas, Neil J. Cook, Nicolas B. Cowan, X. Delfosse, J.-D. do Nascimento, J.‐F. Donati, René Doyon, T. Forveille, P. Fouqué, Eric Gaidos, Emily A. Gilbert, J. Gomes da Silva, J. D. Hartman, Katharine Hesse, Mélissa J. Hobson, Jon M. Jenkins, F. Kiefer, Veselin B. Kostov, J. Laskar, M. Lendl, Alexandrine L’Heureux, J. H. C. Martins, Kristen Menou, C. Moutou, F. Murgas, Alex S. Polanski, David Rapetti, Elyar Sedaghati, Hsien Shang

Bibliographic record

VenueAstronomy and Astrophysics · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsMcGill UniversityUniversity of TorontoMcMaster UniversityUniversité de Montréal
FundersPlanetary Science DivisionInstitut national des sciences de l'UniversFundação para a Ciência e a TecnologiaScience and Technology Facilities CouncilHorizon 2020 Framework ProgrammeH2020 European Research CouncilSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryAgencia Nacional de Investigación y DesarrolloAmes Research CenterCentre National de la Recherche ScientifiqueConselho Nacional de Desenvolvimento Científico e TecnológicoFondo Nacional de Desarrollo Científico y TecnológicoQueen's UniversityAgencia Estatal de InvestigaciónScience Mission DirectorateSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungAgence Nationale de la RechercheSpace Telescope Science InstituteEuropean CommissionMinisterio de Ciencia e InnovaciónMax-Planck-Institut für AstronomieUniversity of EdinburghEötvös Loránd TudományegyetemCalifornia Institute of TechnologyLos Alamos National LaboratoryEuropean Space AgencyJohns Hopkins UniversityEuropean Research CouncilGordon and Betty Moore FoundationQueen's University BelfastNational Science FoundationNational Aeronautics and Space AdministrationNational Central UniversityFundação de Amparo à Pesquisa do Estado de Minas GeraisNuclear Safety and Security CommissionDurham UniversitySmithsonian Institution
KeywordsPhysicsPlanetAstrophysicsOrbital periodExoplanetAstronomyRADIUSRadial velocityStars

Abstract

fetched live from OpenAlex

We report the discovery and characterisation of a giant transiting planet orbiting a nearby M3.5V dwarf (d = 80.4pc, G = 15.1 mag, K=11.2mag, R* = 0.358 ± 0.015 R⊙, M* = 0.340 ± 0.009 M⊙). Using the photometric time series from TESS sectors 10, 36, 46, and 63 and near-infrared spectrophotometry from ExTrA, we measured a planetary radius of 0.77 ± 0.03 RJ and an orbital period of 1.52 days. With high-resolution spectroscopy taken by the CFHT/SPIRou and ESO/ESPRESSO spectrographs, we refined the host star parameters ([Fe/H] = 0.27 ± 0.12) and measured the mass of the planet (0.273 ± 0.006 MJ). Based on these measurements, TOI-4860 b joins the small set of massive planets (>80 ME) found around mid to late M dwarfs (<0.4 R⊙), providing both an interesting challenge to planet formation theory and a favourable target for further atmospheric studies with transmission spectroscopy. We identified an additional signal in the radial velocity data that we attribute to an eccentric planet candidate (e = 0.66 ± 0.09) with an orbital period of 427 ± 7 days and a minimum mass of 1.66 ± 0.26 MJ, but additional data would be needed to confirm this.

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 score0.002
Threshold uncertainty score0.005

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0000.001
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 head0.010
GPT teacher head0.217
Teacher spread0.206 · 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
Published2024
Admission routes2
Has abstractyes

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