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Record W4392775040 · doi:10.1093/mnras/stae508

NGTS-28Ab: a short period transiting brown dwarf

2024· article· en· W4392775040 on OpenAlexfundno aff
Beth A Henderson, S. L. Casewell, M. R. Goad, Jack S Acton, Maximilian N. Günther, Louise D. Nielsen, M. R. Burleigh, Claudia Belardi, Rosanna H Tilbrook, Oliver Turner, Steve B. Howell, Catherine A. Clark, Colin Littlefield, Khalid Barkaoui, D. R. Alves, D. R. Anderson, Daniel Bayliss, F. Bouchy, Edward M. Bryant, George Dransfield, Elsa Ducrot, Philipp Eigmüller, Samuel Gill, Edward Gillen, M. Gillon, Faith Hawthorn, M. J. Hooton, James A. G. Jackman, Emmanuël Jehin, J. S. Jenkins, Alicia Kendall, M. Lendl, J. McCormac, Maximiliano Moyano, P. P. Pedersen, F. J. Pozuelos, Gavin Ramsay, Ramotholo Sefako, Mathilde Timmermans, A. H. M. J. Triaud, S. Udry, José I Vines, C. A. Watson, R. G. West, P. J. Wheatley, Sebastián Zúñiga-Fernández

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersPlanetary Science DivisionScience and Technology Facilities CouncilScience Mission DirectorateAgencia Nacional de Investigación y DesarrolloSmithsonian Astrophysical ObservatoryMax-Planck-Institut für AstronomieKorea Astronomy and Space Science InstituteSpace Telescope Science InstituteMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesEuropean Southern ObservatoryQueen's UniversityNational Aeronautics and Space AdministrationDiabetes Patient Advocacy CoalitionAmes Research CenterLos Alamos National LaboratoryEuropean Space AgencyJohns Hopkins UniversityGordon and Betty Moore FoundationQueen's University BelfastNational Science FoundationEötvös Loránd TudományegyetemCalifornia Institute of TechnologyNational Central UniversityDurham UniversitySmithsonian Institution
KeywordsPhysicsAstronomyBrown dwarfPeriod (music)AstrophysicsStars

Abstract

fetched live from OpenAlex

ABSTRACT We report the discovery of a brown dwarf orbiting a M1 host star. We first identified the brown dwarf within the Next Generation Transit Survey data, with supporting observations found in TESS sectors 11 and 38. We confirmed the discovery with follow-up photometry from the South African Astronomical Observatory, SPECULOOS-S, and TRAPPIST-S, and radial velocity measurements from HARPS, which allowed us to characterize the system. We find an orbital period of ∼1.25 d, a mass of $69.0^{+5.3}_{-4.8}$ MJ, close to the hydrogen burning limit, and a radius of 0.95 ± 0.05 RJ. We determine the age to be >0.5 Gyr, using model isochrones, which is found to be in agreement with spectral energy distribution fitting within errors. NGTS-28Ab is one of the shortest period systems found within the brown dwarf desert, as well as one of the highest mass brown dwarfs that transits an M dwarf. This makes NGTS-28Ab another important discovery within this scarcely populated region.

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 score0.004
Threshold uncertainty score0.009

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 integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.001

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 head0.212
Teacher spread0.203 · 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 routes1
Has abstractyes

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