MétaCan
Menu
← Back to cohort
Record W2186599455 · doi:10.3847/0004-637x/816/2/95

THE KEPLER-454 SYSTEM: A SMALL, NOT-ROCKY INNER PLANET, A JOVIAN WORLD, AND A DISTANT COMPANION

2016· article· en· W2186599455 on OpenAlexfundno aff
Sara Gettel, David Charbonneau, Courtney D. Dressing, Lars A. Buchhave, X. Dumusque, Andrew Vanderburg, A. S. Bonomo, L. Malavolta, F. Pepe, A. Collier Cameron, David W. Latham, S. Udry, Geoffrey W. Marcy, Howard Isaacson, Andrew W. Howard, G. R. Davies, V. Silva Aguirre, H. Kjeldsen, Eric Lopez, L. Affer, R. Cosentino, P. Figueira, A. F. Martínez Fiorenzano, A. Harutyunyan, John Asher Johnson, Mercedes López‐Morales, C. Lovis, M. Mayor, E. Molinari, F. Motalebi, David F. Phillips, G. Piotto, D. Queloz, Ken Rice, Dimitar Sasselov, D. Ségransan, A. Sozzetti, Chris Watson, Sarbani Basu, T. L. Campante, J. Christensen‐Dalsgaard, S. D. Kawaler, Τ. S. Metcalfe, R. Handberg, Mikkel N. Lund, M. Lundkvist, Daniel Huber, W. J. Chaplin

Bibliographic record

VenueThe Astrophysical Journal · 2016
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersScience Mission DirectorateSmithsonian Astrophysical ObservatoryUniversité de GenèveDanmarks GrundforskningsfondScience and Technology Facilities CouncilNational Research FoundationQueen's University BelfastUniversity of St AndrewsScottish Universities Physics AllianceStellar Astrophysics CentreQueen's UniversitySchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungNASA Exoplanet Science InstituteFundação para a Ciência e a TecnologiaHarvard UniversityJohn Templeton FoundationW. M. Keck FoundationEuropean CommissionCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationSmithsonian InstitutionNational Science Foundation
KeywordsPhysicsPlanetAstrophysicsExoplanetAstronomyRadial velocityPlanetary systemRADIUSPlanetary massSpectrographStarsSpectral line

Abstract

fetched live from OpenAlex

ABSTRACT Kepler-454 (KOI-273) is a relatively bright (V = 11.69 mag), Sun-like star that hosts a transiting planet candidate in a 10.6 day orbit. From spectroscopy, we estimate the stellar temperature to be 5687 ± 50 K, its metallicity to be [m/H] = 0.32 ± 0.08, and the projected rotational velocity to be v sin i < 2.4 km s−1. We combine these values with a study of the asteroseismic frequencies from short cadence Kepler data to estimate the stellar mass to be , the radius to be 1.066 ± 0.012 R ⊙, and the age to be Gyr. We estimate the radius of the 10.6 day planet as 2.37 ± 0.13 R ⊕. Using 63 radial velocity observations obtained with the HARPS-N spectrograph on the Telescopio Nazionale Galileo and 36 observations made with the HIRES spectrograph at the Keck Observatory, we measure the mass of this planet to be 6.8 ± 1.4 M ⊕. We also detect two additional non-transiting companions, a planet with a minimum mass of 4.46 ± 0.12 M J in a nearly circular 524 day orbit and a massive companion with a period >10 years and mass >12.1 M J . The 12 exoplanets with radii <2.7 R ⊕ and precise mass measurements appear to fall into two populations, with those <1.6 R ⊕ following an Earth-like composition curve and larger planets requiring a significant fraction of volatiles. With a density of 2.76 ± 0.73 g cm−3, Kepler-454b lies near the mass transition between these two populations and requires the presence of volatiles and/or H/He gas.

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 score0.009

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 communication0.0010.001
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

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 head0.011
GPT teacher head0.203
Teacher spread0.191 · 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

Citations42
Published2016
Admission routes1
Has abstractyes

Explore more

Same venueThe Astrophysical Journal→Same topicStellar, planetary, and galactic studies→French-language works237,207→