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Record W4415415233 · doi:10.1093/mnras/staf1806

An ultra-short period super-Earth and sub-Neptune spanning the Radius Valley orbiting the kinematic thick disc star TOI-2345

2025· article· en· W4415415233 on OpenAlexfundno aff
Yoshi Nike Emilia Eschen, T. G. Wilson, A. Bonfanti, C. M. Persson, S. G. Sousa, M. Lendl, A. Heitzmann, A. E. Simon, G. Olofsson, A. Castro-González, J. A. Egger, L. Fossati, Alexander J. Mustill, H. P. Osborn, H. G. Vivien, Y. Alibert, R. Alonso, T. Bárczy, D. Barrado, S. C. C. Barros, W. Baumjohann, W. Benz, N. Billot, L. Borsato, A. Brandeker, C. Broeg, Maximilian Buder, Douglas A. Caldwell, A. Collier Cameron, A. C. M. Correia, Szilárd Csizmadia, Patricio E. Cubillos, M. B. Davies, Magali Deleuil, A. Deline, O. D. S. Demangeon, Brice-Olivier Demory, A. Derekas, Billy Edwards, D. Ehrenreich, A. Erikson, Jacopo Farinato, A. Fortier, M. Fridlund, D. Gandolfi, K. Gazeas, M. Gillon, Robert F. Goeke, M. Guêdel, Maximilian N. Günther, J. Hasiba, Ch. Helling, K. Isaak, Jon M. Jenkins, T. Keller, L. L. Kiss, Daniel Kitzmann, J. Korth, K. W. F. Lam, J. Laskar, A. Lecavelier des Étangs, Adrien Leleu, Demetrio Magrin, P. F. L. Maxted, B. Merín, Christoph Mordasini, V. Nascimbeni, R. Ottensamer, Isabella Pagano, Ε. Πάλλη, G. Peter, D. Piazza, G. Piotto, D. Pollacco, D. Queloz, Roberto Ragazzoni, N. Rando, F. Ratti, H. Rauer, I. Ribas, N. C. Santos, D. Ségransan, Avi Shporer, A. M. S. Smith, M. Stalport, S. Sulis, Gyula M. Szabó, S. Udry, Soléne Ulmer-Moll, J. Venturini, Eva Villaver, N. A. Walton, David Watanabe, S. Wolf, Carl Ziegler

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersNuclear Fuel Cycle and Supply ChainEuropean Regional Development FundStaatssekretariat für Bildung, Forschung und InnovationScience and Technology Facilities CouncilHorizon 2020 Framework ProgrammeInstituto de Astrofísica de CanariasFundação para a Ciência e a TecnologiaCentre National d’Etudes SpatialesFonds De La Recherche Scientifique - FNRSUK Space AgencyAustrian Science FundSwedish National Space AgencyNational Research, Development and Innovation OfficeAgencia Estatal de InvestigaciónScience Mission DirectorateSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungCanadian Celiac AssociationAgence Nationale de la RechercheInstitut Universitaire de FranceUniversity of WarwickDeutsche ForschungsgemeinschaftCentres de Recerca de CatalunyaNational Science FoundationUK Research and InnovationNational Aeronautics and Space AdministrationMinisterio de Ciencia e InnovaciónEuropean CommissionFondazione CRTEuropean Space AgencyNemzeti Kutatási Fejlesztési és Innovációs HivatalCalifornia Institute of TechnologyGeneralitat de CatalunyaSpine Education and Research InstituteSimons Foundation
KeywordsExoplanetPlanetRADIUSStarsPlanetary systemKinematicsPeriod (music)Mass distribution

Abstract

fetched live from OpenAlex

ABSTRACT A crucial chemical link between stars and their orbiting exoplanets is thought to exist. If universal, this connection could affect the formation and evolution of all planets. Therefore, this potential vital link needs testing by characterizing exoplanets around chemically-diverse stars. We present the discovery of two planets orbiting the metal-poor, kinematic thick-disc K-dwarf TOI-2345. TOI-2345 b is a super-Earth with a period of 1.05 d and TOI-2345 c is a sub-Neptune with a period of 21 d. In addition to the target being observed in four TESS sectors, we obtained five CHEOPS visits and 26 radial velocities from HARPS. By conducting a joint analysis of all the data, we find TOI-2345 b to have a radius of $1.504\substack{+0.047 -0.044}$ R$_{\oplus }$ and a mass of $3.49\pm 0.85$ M$_{\oplus }$; and TOI-2345 c to have a radius of $2.451\substack{+0.045 -0.046}$ R$_{\oplus }$ and a mass of $7.27\substack{+2.27 -2.45}$ M$_{\oplus }$. To explore chemical links between these planets and their host star, we model their interior structures newly accounting for devolatized stellar abundances. TOI-2345 adds to the limited sample of well-characterized planetary systems around thick disc stars. This system challenges theories of formation and populations of planets around thick disc stars with its Ultra-Short Period super-Earth and the wide period distribution of these two planets spanning the radius valley.

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 score0.013
Threshold uncertainty score0.026

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
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 head0.008
GPT teacher head0.213
Teacher spread0.205 · 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

Citations1
Published2025
Admission routes1
Has abstractyes

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