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Record W2909256704 · doi:10.1093/mnras/stz139

K2-290: a warm Jupiter and a mini-Neptune in a triple-star system

2019· article· en· W2909256704 on OpenAlexfundno aff
María Hjorth, A. B. Justesen, Teruyuki Hirano, Simon Albrecht, D. Gandolfi, F. Dai, R. Alonso, Oscar Barragán, M. Esposito, Masayuki Kuzuhara, K. W. F. Lam, John H. Livingston, P. Montañés‐Rodríguez, Norio Narita, G. Nowak, J. Prieto-Arranz, Seth Redfield, F. Rodler, Joshua N. Winn, G. Antoniciello, J. Cabrera, William D. Cochran, Sz. Csizmadia, H. J. Deeg, Philipp Eigmüller, Michael Endl, A. Erikson, M. Fridlund, S. Grziwa, E. W. Guenther, A. P. Hatzes, Paul Heeren, D. Hidalgo, J. Korth, R. Luque, D. Nespral, Ε. Πάλλη, M. Pätzold, C. M. Persson, H. Rauer, A. M. S. Smith, Trifon Trifonov

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsnot available
FundersJapan Society for the Promotion of ScienceScience Mission DirectorateIstituto Nazionale di AstrofisicaEuropean School of OncologySpace Telescope Science InstituteAssociation of Canadian Universities for Research in AstronomyEuropean CommissionStellar Astrophysics CentreHorizon 2020National Astronomical Observatory of JapanDanmarks GrundforskningsfondDanmarks Frie ForskningsfondNational Science FoundationEuropean Space AgencyNational Aeronautics and Space AdministrationDeutsche ForschungsgemeinschaftScience and Technology Facilities CouncilNational Research Foundation
KeywordsPhysicsNeptuneAstronomyJupiter (rocket family)Star (game theory)AstrophysicsAstrobiologyPlanetSpacecraft

Abstract

fetched live from OpenAlex

We report the discovery of two transiting planets orbiting K2-290 (EPIC 249624646), a bright (V = 11.11) late F-type star residing in a triple-star system. It was observed during Campaign 15 of the K2 mission, and in order to confirm and characterize the system, follow-up spectroscopy and AO imaging were carried out using the FIES, HARPS, HARPS-N, and IRCS instruments. From AO imaging and Gaia data we identify two M-dwarf companions at a separation of 113 ± 2 and 246-155+177 au. From radial velocities, K2 photometry, and stellar characterization of the host star, we find the inner planet to be a mini-Neptune with a radius of 3.06 ± 0.16 R⊕ and an orbital period of P = 9.2 d. The radius of the mini-Neptune suggests that the planet is located above the radius valley, and with an incident flux of F ~ 400 F⊕, it lies safely outside the super-Earth desert. The outer warm Jupiter has a mass of 0.774 ± 0.047 MJ and a radius of 1.006 ± 0.050 RJ, and orbits the host star every 48.4 d on an orbit with an eccentricity e < 0.241. Its mild eccentricity and mini-Neptune sibling suggest that the warm Jupiter originates from in situ formation or disc migration.

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: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.389
Threshold uncertainty score0.528

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 studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
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 head0.005
GPT teacher head0.177
Teacher spread0.173 · 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 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

Citations36
Published2019
Admission routes1
Has abstractyes

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