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Record W3042845680 · doi:10.1093/mnras/staa2077

K2-280 b – a low density warm sub-Saturn around a mildly evolved star

2020· article· en· W3042845680 on OpenAlexfundno aff
G. Nowak, Ε. Πάλλη, D. Gandolfi, H. J. Deeg, Teruyuki Hirano, Oscar Barragán, Masayuki Kuzuhara, Fei Dai, R. Luque, C. M. Persson, M. Fridlund, Marshall C. Johnson, J. Korth, John H. Livingston, S. Grziwa, S. Mathur, A. P. Hatzes, J. Prieto-Arranz, D. Nespral, D. Hidalgo, María Hjorth, Simon Albrecht, Vincent Van Eylen, K. W. F. Lam, William D. Cochran, M. Esposito, Szilárd Csizmadia, E. W. Guenther, P. Kábath, P. Blay, Rafael Brahm, Andrés Jordán, Néstor Espinoza, Felipe Rojas, Núria Casasayas Barris, F. Rodler, Roi Alonso Sobrino, I. Carleo, Alexander Chaushev, Jerome de Leon, Philipp Eigmüller, Michael Endl, A. Erikson, Akihiko Fukui, Iskra Georgieva, Lucía González-Cuesta, Emil Knudstrup, Mikkel N. Lund, P. Montañés‐Rodríguez, F. Murgas, Norio Narita, Prajwal Niraula, M. Pätzold, H. Rauer, Seth Redfield, I. Ribas, M. Skarka, A. M. S. Smith, Jano Subjak

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersPrecursory Research for Embryonic Science and TechnologyFondo Nacional de Desarrollo Científico y TecnológicoComisión Nacional de Investigación Científica y TecnológicaJapan Society for the Promotion of ScienceInstitut sur la Nutrition et les Aliments FonctionnelsMinisterio de Economía, Fomento y Turismo, ChileScience and Technology Facilities CouncilNational Research Council CanadaInstituto de Astrofísica de CanariasKorea Astronomy and Space Science InstituteMinistério da Ciência, Tecnologia e InovaçãoJapan Science and Technology CorporationDeutsche ForschungsgemeinschaftMinisterio de Ciencia, Tecnología e Innovación ProductivaIstituto Nazionale di AstrofisicaMinisterio de Economía y CompetitividadSwedish National Space AgencyNational Science Foundation
KeywordsPhysicsAstrophysicsPlanetSaturnRadial velocityRADIUSStar (game theory)Surface gravityAstronomyStars

Abstract

fetched live from OpenAlex

ABSTRACT We present an independent discovery and detailed characterization of K2-280 b, a transiting low density warm sub-Saturn in a 19.9-d moderately eccentric orbit (e = $0.35_{-0.04}^{+0.05}$ ) from K2 campaign 7. A joint analysis of high precision HARPS, HARPS-N, and FIES radial velocity measurements and K2 photometric data indicates that K2-280 b has a radius of Rb = 7.50 ± 0.44 R⊕ and a mass of Mb = 37.1 ± 5.6 M⊕, yielding a mean density of ρb = $0.48 _{ - 0.10 } ^ { + 0.13 }$ ${\rm g\, cm^{-3}}$. The host star is a mildly evolved G7 star with an effective temperature of Teff = 5500 ± 100 K, a surface gravity of $\log \, g_{\star }$ = 4.21 ± 0.05 (cgs), and an iron abundance of [Fe/H] = ${0.33}\, {\pm }\, {0.08}$ dex, and with an inferred mass of M⋆ = 1.03 ± 0.03 M⊙ and a radius of R⋆ = 1.28 ± 0.07 R⊙. We discuss the importance of K2-280 b for testing formation scenarios of sub-Saturn planets and the current sample of this intriguing group of planets that are absent in the Solar system.

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 score0.007
Threshold uncertainty score0.013

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 science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.192
Teacher spread0.182 · 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

Citations8
Published2020
Admission routes1
Has abstractyes

Explore more

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