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Record W4415272861 · doi:10.48550/arxiv.2510.12783

An Ultra-Short Period Super-Earth and Sub-Neptune Spanning the Radius Valley Orbiting the Kinematic Thick Disk Star TOI-2345

2025· preprint· en· W4415272861 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, Szilard 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, Michaël Gillon, Robert F. Goeke, M. Güdel, Maximilian N. Günther, J. Hasiba, Ch. Helling, K. G. 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, Valerio Nascimbeni, R. Ottensamer, Isabella Pagano, Ε. Πάλλη, G. Peter, D. Piazza, G. Piotto, D. Pollacco, D. Queloz, Roberto Ragazzoni, N. Rando, F. Ratti, Heike Rauer, I. Ribas, N. C. Santos, Damien Ségransan, Avi Shporer, A. M. S. Smith, M. Stalport, S. Sulis, Gyula M. Szabó, S. Udry, Soléne Ulmer-Moll, V. Van Grootel, J. Venturini, Eva Villaver, N. A. Walton, David Watanabe, S. Wolf, Carl Ziegler

Bibliographic record

VenueArXiv.org · 2025
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersEuropean Regional Development FundStaatssekretariat für Bildung, Forschung und InnovationInstituto de Astrofísica de CanariasFundação para a Ciência e a TecnologiaCentre National d’Etudes SpatialesFondazione CRTEuropean CommissionMinisterio de Ciencia e InnovaciónGeneralitat de CatalunyaFonds De La Recherche Scientifique - FNRSUK Space AgencyAustrian Science FundSwedish National Space AgencyAgencia Estatal de InvestigaciónScience Mission DirectorateSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungCanadian Celiac AssociationAgence Nationale de la RechercheCalifornia Institute of TechnologyInstitut Universitaire de FranceUniversity of WarwickDeutsche ForschungsgemeinschaftCentres de Recerca de CatalunyaNational Science FoundationUK Research and InnovationScience and Technology Facilities CouncilHorizon 2020 Framework ProgrammeEuropean Space AgencyNational Aeronautics and Space Administration
KeywordsExoplanetPlanetRADIUSStarsPlanetary systemKinematicsPeriod (music)Star (game theory)

Abstract

fetched live from OpenAlex

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 characterising exoplanets around chemically-diverse stars. We present the discovery of two planets orbiting the metal-poor, kinematic thick-disk K-dwarf TOI-2345. TOI-2345 b is a super-Earth with a period of 1.05 days and TOI-2345 c is a sub-Neptune with a period of 21 days. In addition to the target being observed in 4 TESS sectors, we obtained 5 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 $3.49\pm0.85$ 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 devolatised stellar abundances. TOI-2345 adds to the limited sample of well characterised planetary systems around thick disk stars. This system challenges theories of formation and populations of planets around thick disk 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 score0.012
Threshold uncertainty score0.024

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 head0.027
GPT teacher head0.254
Teacher spread0.227 · 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

Citations0
Published2025
Admission routes1
Has abstractyes

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