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Record W3085377485 · doi:10.1051/0004-6361/202039455

A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776

2020· article· en· W3085377485 on OpenAlexaff

Bibliographic record

VenueAstronomy and Astrophysics · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversity of Toronto
FundersPrecursory Research for Embryonic Science and TechnologyJapan Society for the Promotion of ScienceCollege of Engineering, Michigan State UniversityMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesDanmarks GrundforskningsfondDeutsche ForschungsgemeinschaftScience and Technology Facilities CouncilMichigan State UniversityNational Research FoundationKorea Astronomy and Space Science InstituteFondazione CRTMinistério da Ciência, Tecnologia e InovaçãoUniversity of North Carolina at Chapel HillEuropean CommissionStellar Astrophysics CentreAgencia Nacional de Investigación y DesarrolloSwedish National Space AgencyDanmarks Frie ForskningsfondNational Science Foundation
KeywordsExoplanetPlanetRADIUSPhotometry (optics)Planetary systemStarsTransit (satellite)Radial velocityLow Mass

Abstract

fetched live from OpenAlex

We report the discovery and characterization of two transiting planets around the bright M1 V star LP 961-53 (TOI-776,J= 8.5 mag,M= 0.54 ± 0.03M⊙) detected during Sector 10 observations of the Transiting Exoplanet Survey Satellite (TESS). Combining the TESS photometry with HARPS radial velocities, as well as ground-based follow-up transit observations from the MEarth and LCOGT telescopes, for the inner planet, TOI-776 b, we measured a period ofPb= 8.25 d, a radius ofRb= 1.85 ± 0.13R⊕, and a mass ofMb= 4.0 ± 0.9M⊕; and for the outer planet, TOI-776 c, a period ofPc= 15.66 d, a radius ofRc= 2.02 ± 0.14R⊕, and a mass ofMc= 5.3 ± 1.8M⊕. The Doppler data shows one additional signal, with a period of ~34 d, associated with the rotational period of the star. The analysis of fifteen years of ground-based photometric monitoring data and the inspection of different spectral line indicators confirm this assumption. The bulk densities of TOI-776 b and c allow for a wide range of possible interior and atmospheric compositions. However, both planets have retained a significant atmosphere, with slightly different envelope mass fractions. Thanks to their location near the radius gap for M dwarfs, we can start to explore the mechanism(s) responsible for the radius valley emergence around low-mass stars as compared to solar-like stars. While a larger sample of well-characterized planets in this parameter space is still needed to draw firm conclusions, we tentatively estimate that the stellar mass below which thermally-driven mass loss is no longer the main formation pathway for sculpting the radius valley is between 0.63 and 0.54M⊙. Due to the brightness of the star, the TOI-776 system is also an excellent target for theJames WebbSpace Telescope, providing a remarkable laboratory in which to break the degeneracy in planetary interior models and to test formation and evolution theories of small planets around low-mass stars.

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
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0000.001
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 head0.009
GPT teacher head0.180
Teacher spread0.172 · 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

Citations51
Published2020
Admission routes1
Has abstractyes

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