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Record W3089044629 · doi:10.1093/mnras/stab1567

Discovery of a young low-mass brown dwarf transiting a fast-rotating F-type star by the Galactic Plane eXoplanet (GPX) survey

2021· preprint· en· W3089044629 on OpenAlexaff
Paul Benni, Artem Burdanov, V. Krushinsky, A. Bonfanti, G. Hébrard, J. M. Almenara, S. Dalal, O. D. S. Demangeon, M. Tsantaki, Joshua Pepper, Keivan G. Stassun, Andrew Vanderburg, A. Belinski, F. V. Kashaev, Khalid Barkaoui, T. Kim, Wonseok Kang, K. A. Antonyuk, V. V. Dyachenko, Д. А. Растегаев, A. Beskakotov, А. А. Митрофанова, F. J. Pozuelos, A. Popov, F. Kiefer, P. A. Wilson, G. Ricker, R. Vanderspek, David W. Latham, Sara Seager, Jon M. Jenkins, E. Sokov, I. Sokova, Alessandro Marchini, Riccardo Papini, Fabio Salvaggio, Massimo Banfi, Özgür Baştürk, Ş. Torun, Selçuk Yalçınkaya, K. Ivanov, G. G. Valyavin, Emmanuël Jehin, M. Gillon, E. Pakštienė, Stan Shadick, M. Bretton, A. Wünsche, J. Garlitz, Y. Jongen, D. Molina, Éric Girardin, R. Naves, Z. Benkhaldoun, M. D. Joner, M. Spencer, Allyson Bieryla, Daniel J. Stevens, Eric L. N. Jensen, Karen A. Collins, David Charbonneau, Elisa V. Quintana, Susan E. Mullally, Christopher E. Henze

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversity of Saskatchewan
FundersFundação para a Ciência e a TecnologiaScience Mission DirectorateHorizon 2020 Framework ProgrammeLomonosov Moscow State UniversityUniversité Cadi AyyadRussian Science FoundationTürkiye Bilimsel ve Teknolojik Araştırma KurumuCalifornia Institute of TechnologyEuropean CommissionFondazione Internazionale Premio BalzanFonds De La Recherche Scientifique - FNRSScience and Technology Facilities CouncilMississippi State UniversityAmes Research CenterMinistry of Science and Higher Education of the Russian FederationFédération Wallonie-BruxellesIrkutsk State UniversityNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsPhysicsBrown dwarfAstrophysicsExoplanetLow MassStar (game theory)Effective temperatureGalactic planePlanetRADIUSOrbital planeAstronomyStars

Abstract

fetched live from OpenAlex

ABSTRACT We announce the discovery of GPX-1 b, a transiting brown dwarf with a mass of 19.7 ± 1.6 MJup and a radius of 1.47 ± 0.10 RJup, the first substellar object discovered by the Galactic Plane eXoplanet (GPX) survey. The brown dwarf transits a moderately bright (V = 12.3 mag) fast-rotating F-type star with a projected rotational velocity $v\sin {\, i_*}=40\pm 10$ km s−1. We use the isochrone placement algorithm to characterize the host star, which has effective temperature 7000 ± 200 K, mass 1.68 ± 0.10 $\mathrm{\it M}_\odot$, radius 1.56 ± 0.10 $\mathrm{\it R}_\odot$, and approximate age $0.27_{-0.15}^{+0.09}$ Gyr. GPX-1 b has an orbital period of ∼1.75 d and a transit depth of 0.90 ± 0.03 per cent. We describe the GPX transit detection observations, subsequent photometric and speckle-interferometric follow-up observations, and SOPHIE spectroscopic measurements, which allowed us to establish the presence of a substellar object around the host star. GPX-1 was observed at 30-min integrations by TESS in Sector 18, but the data are affected by blending with a 3.4 mag brighter star 42 arcsec away. GPX-1 b is one of about two dozen transiting brown dwarfs known to date, with a mass close to the theoretical brown dwarf/gas giant planet mass transition boundary. Since GPX-1 is a moderately bright and fast-rotating star, it can be followed-up by the means of the Doppler tomography.

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 score0.005

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.012
GPT teacher head0.212
Teacher spread0.200 · 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
Published2021
Admission routes1
Has abstractyes

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