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Record W2888480245 · doi:10.1093/mnras/sty2360

K2-263 b: a 50 d period sub-Neptune with a mass measurement using HARPS-N

2018· article· en· W2888480245 on OpenAlexfundno aff
Annelies Mortier, A. S. Bonomo, Vinesh Rajpaul, Lars A. Buchhave, Andrew Vanderburg, Li Zeng, Mercedes López‐Morales, L. Malavolta, A. Collier Cameron, Courtney D. Dressing, P. Figueira, V. Nascimbeni, Ken Rice, A. Sozzetti, C. A. Watson, L. Affer, F. Bouchy, David Charbonneau, A. Harutyunyan, R. D. Haywood, John Asher Johnson, David W. Latham, C. Lovis, A. F. Martínez Fiorenzano, M. Mayor, G. Micela, E. Molinari, F. Motalebi, F. Pepe, G. Piotto, David F. Phillips, E. Poretti, Dimitar Sasselov, D. Ségransan, S. Udry

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsnot available
FundersSeventh Framework ProgrammeScience and Technology Facilities CouncilSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryUniversité de GenèveScience Mission DirectorateIstituto Nazionale di AstrofisicaQueen's University BelfastUniversity of St AndrewsScottish Universities Physics AllianceRoyal Astronomical SocietyQueen's UniversitySchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungNASA Exoplanet Science InstituteSpace Telescope Science InstituteHarvard UniversityNational Aeronautics and Space AdministrationEuropean CommissionCalifornia Institute of TechnologyJohn Templeton FoundationSmithsonian InstitutionNational Science Foundation
KeywordsPhysicsNeptuneAstronomyAstrophysicsPeriod (music)Planet

Abstract

fetched live from OpenAlex

This paper reports on the validation and mass measurement of EPIC211682544b, a sub-Neptune orbiting a quiet G9V star. Using K2 data from campaigns C5 and C16, we find this planet to have a period of$50.818947\pm 0.000094$ days and a radius of $2.41\pm0.12$ R$_{\oplus}$.We followed this system with HARPS-N to obtain 67 precise radial velocities. A combined fit of the transit and radial velocity data reveals that EPIC211682544b has a mass of $14.8\pm3.1$ M$_{\oplus}$. Its bulk density ($5.7_{-1.4}^{+1.6}$ g cm$^{-3}$) implies that this planet has a significant envelope of water or other volatiles around a rocky core. EPIC211682544b likely formed in a similar way as the cores of the four giant planets in our own Solar System, but for some reason, did not accrete much gas. The planetary mass was confirmed by an independent Gaussian process-based fit to both the radial velocities and the spectroscopic activity indicators. EPIC211682544b belongs to only a handful of confirmed K2 exoplanets with periods longer than 40 days. Itis among the longest periods for a small planet with a precisely determined mass using radial velocities.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.276
Threshold uncertainty score0.629

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.001
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.015
GPT teacher head0.195
Teacher spread0.180 · 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 teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
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

Citations17
Published2018
Admission routes1
Has abstractyes

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