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Record W4225758506 · doi:10.1093/mnras/stac1448

<i>TESS</i> discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136

2022· article· en· W4225758506 on OpenAlexaffabout
Tianjun Gan, Abderahmane Soubkiou, Sharon X. Wang, Z. Benkhaldoun, Shude Mao, Étienne Artigau, P. Fouqué, L. Arnold, Steven Giacalone, Christian Aganze, Adam J. Burgasser, Karen A. Collins, Avi Shporer, Khalid Barkaoui, Mourad Ghachoui, Steve B. Howell, C. Lamman, O. D. S. Demangeon, Artem Burdanov, Charles Cadieux, J. Chouqar, Kevin I. Collins, Neil J. Cook, L. Delrez, Brice-Olivier Demory, René Doyon, Georgina Dransfield, Courtney D. Dressing, Elsa Ducrot, Jiahao Fan, L. J. Garcia, Holden Gill, M. Gillon, Crystal L. Gnilka, Maximilian N. Günther, Christopher E. Henze, Chelsea X. Huang, Emmanuël Jehin, Eric L. N. Jensen, Zitao Lin, N. Manset, J. McCormac, C. A. Murray, Prajwal Niraula, P.P. Pedersen, F. J. Pozuelos, D. Queloz, Benjamin V. Rackham, Arjun B Savel, N. Schanche, Richard P. Schwarz, Daniel Sebastian, Samantha Thompson, Mathilde Timmermans, A. H. M. J. Triaud, M. Vezie, Robert D. Wells, Julien de Wit, G. Ricker, R. Vanderspek, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversité de MontréalUniversité du Québec à Montréal
FundersErasmus+European Regional Development FundNational Institutes of Natural SciencesFundação para a Ciência e a TecnologiaSeventh Framework ProgrammeAgencia Nacional de Investigación y DesarrolloUniversité Cadi AyyadAustralian Research CouncilKorea Astronomy and Space Science InstituteUniversidad Nacional Autónoma de MéxicoMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesScience and Technology Facilities CouncilHorizon 2020 Framework ProgrammeFonds pour la Formation à la Recherche dans l’Industrie et dans l’AgricultureUniversidade do PortoAmes Research CenterFédération Wallonie-BruxellesHeising-Simons FoundationFonds De La Recherche Scientifique - FNRSMinistry of Science, ICT and Future PlanningScience Mission DirectorateSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungSimons FoundationUniversité de LiègePrecursory Research for Embryonic Science and TechnologyCalifornia Institute of TechnologyEuropean CommissionFondation MeracNational Science FoundationEuropean Space AgencyNational Aeronautics and Space AdministrationNational Natural Science Foundation of ChinaJapan Society for the Promotion of ScienceNational Geographic Society
KeywordsPhysicsPhotometry (optics)NeptunePlanetAstrophysicsRADIUSAstronomyStarsEffective temperatureExoplanetBrown dwarf

Abstract

fetched live from OpenAlex

ABSTRACT We present the discovery of TOI-2136 b, a sub-Neptune planet transiting a nearby M4.5V-type star every 7.85 d, identified through photometric measurements from the Transiting Exoplanet Survey Satellite (TESS) mission. The host star is located 33 pc away with a radius of R* = 0.34 ± 0.02 R⊙, a mass of $0.34\pm 0.02 \, \mathrm{M}_{\odot }$, and an effective temperature of 3342 ± 100 K. We estimate its stellar rotation period to be 75 ± 5 d based on archival long-term photometry. We confirm and characterize the planet based on a series of ground-based multiwavelength photometry, high-angular-resolution imaging observations, and precise radial velocities from Canada–France–Hawaii Telescope (CFHT)/SpectroPolarimètre InfraROUge (SPIRou). Our joint analysis reveals that the planet has a radius of 2.20 ± 0.17 R⊕ and a mass of 6.4 ± 2.4 M⊕. The mass and radius of TOI-2136 b are consistent with a broad range of compositions, from water-ice to gas-dominated worlds. TOI-2136 b falls close to the radius valley for M dwarfs predicted by thermally driven atmospheric mass-loss models, making it an interesting target for future studies of its interior structure and atmospheric properties.

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 score0.004

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 communication0.0010.000
Open science0.0000.001
Research integrity0.0010.000
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 head0.008
GPT teacher head0.195
Teacher spread0.187 · 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

Citations21
Published2022
Admission routes2
Has abstractyes

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