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Record W4408016160 · doi:10.1051/0004-6361/202452916

TOI-2015 b: A sub-Neptune in strong gravitational interaction with an outer non-transiting planet

2025· article· en· W4408016160 on OpenAlexaff
Khalid Barkaoui, J. Korth, E. Gaidos, E. Agol, H. Parviainen, F. J. Pozuelos, E. Palle, Norio Narita, Simon L. Grimm, M. Brady, J.L. Bean, Giuseppe Morello, Benjamin V. Rackham, Adam J. Burgasser, V. Van Grootel, B. Rojas-Ayala, A. Seifahrt, E. Marfil, V. M. Passegger, M. Stalport, M. Gillon, K.A. Collins, A. Shporer, S. Giacalone, Selçuk Yalçınkaya, Elsa Ducrot, Mathilde Timmermans, A.H.M.J. Triaud, J. de Wit, A. Soubkiou, Cristilyn N. Watkins, Christian Aganze, R. Alonso, P. J. Amado, Ritvik Basant, Özgür Baştürk, Z. Benkhaldoun, Artem Burdanov, Y. Calatayud-Borras, J. Chouqar, D.M. Conti, K.I. Collins, Fatemeh Davoudi, L. Delrez, C.D. Dressing, Jerome de Leon, M. Dévora-Pajares, B. -O. Demory, G. Dransfield, E. Esparza-Borges, Gareb Fernández-Rodríguez, Izuru Fukuda, Akihiko Fukui, Pedro Pablo Meni Gallardo, L. J. Garcia, Néstor Abreu García, M. Ghachoui, S. Geraldía-González, Y. Gómez Maqueo Chew, Josafat González-Rodríguez, Maximilian N. Günther, Yuya Hayashi, K. Horne, M. J. Hooton, Kai Ikuta, K. Isogai, E. Jehin, J.M. Jenkins, Kiyoe Kawauchi, Taiki Kagetani, Y. Kawai, David C. Kasper, J.F. Kielkopf, P. Klagyivik, G. Lacedelli, D.W. Latham, Florence Libotte, R. Luque, J.H. Livingston, L. Mancini, B. Massey, M. Mori, S. Muñoz Torres, F. Murgas, Prajwal Niraula, J. Orell-Miquel, David Rapetti, R. Rebolo-Lopez, G. Ricker, R. Papini, P.P. Pedersen, A. Peláez-Torres, J. A. Pérez-Prieto, E. Poultourtzidis, Pablo M. Rodríguez, D. Queloz, Arjun B. Savel, N. Schanche, M. Sánchez-Benavente, L.R. Sibbald, R. Sefako, S. Sohy, A. Sota, R.P. Schwarz, S. Seager, Daniel Sebastian, J. Southworth, M. Stangret, G. Stefansson, J. Sturmer, G. Srdoc, Samantha Thompson, Y. Terada, R. Vanderspek, G. Wang, N. Watanabe, Francis P. Wilkin, J. Winn, Robert D. Wells, C. Ziegler, Sebastián Zúñiga-Fernández

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsRoyal Astronomical Society of Canada
Fundersnot available
KeywordsPhysicsPlanetNeptuneAstrophysicsAstronomyGravitationOuter planetsAstrobiology

Abstract

fetched live from OpenAlex

TOI-2015 is a known exoplanetary system around an M4 dwarf star, consisting of a transiting sub-Neptune planet in a 3.35-day orbital period, TOI-2015 b, accompanied by a non-transiting companion, TOI-2015 c. High-precision radial-velocity measurements were taken with the MAROON-X spectrograph, and high-precision photometric data were collected, primarily using the SPECULOOS, MUSCAT, TRAPPIST and LCOGT networks. We collected 63 transit light curves and 49 different transit epochs for TOI-2015 b. We recharacterized the target star by combining optical spectra obtained by the MAROON-X, Shane/KAST and IRTF/SpeX spectrographs, Bayesian model averaging (BMA) and spectral energy distribution (SED) analysis. The TOI-2015 host star is a K = 10.3 mag M4-type dwarf with a subsolar metallicity of [Fe/H] = −0.31 ± 0.16, and an effective temperature of T eff ≈ 3200 K. Our photodynamical analysis of the system strongly favors the 5:3 mean-motion resonance and in this scenario the planet b (TOI-2015 b) has an orbital period of P b = 3.34 days, a mass of M p = 9.02 -0.36 +0.32 M ⊕ , and a radius of R p = 3.309 -0.011 +0.013 R ⊕ , resulting in a density of ρ p = 0.25 ± 0.01 ρ ⊕ = 1.40 ± 0.06 g cm −3 ; this is indicative of a Neptune-like composition. Its transits exhibit large (> 1 hr) timing variations characteristic of an outer perturber in the system. We performed a global analysis of the high-resolution radial-velocity measurements, the photometric data, and the TTVs, and inferred that TOI-2015 hosts a second planet, TOI-2015 c, in a non-transiting configuration. Our analysis places it near a 5:3 resonance with an orbital period of P c = 5.583 days and a mass of M p = 8.91 -0.40 +0.38 M ⊕ . The dynamical configuration of TOI-2015 b and TOI-2015 c can be used to constrain the system’s planetary formation and migration history. Based on the mass-radius composition models, TOI-2015 b is a water-rich or rocky planet with a hydrogen-helium envelope. Moreover, TOI-2015 b has a high transmission-spectroscopic metric (TSM=149), making it a favorable target for future transmission spectroscopic observations with the JWST to constrain the atmospheric composition of the planet. Such observations would also help to break the degeneracies in theoretical models of the planet’s interior structure.

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 score0.008
Threshold uncertainty score0.015

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 communication0.0000.000
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 head0.005
GPT teacher head0.220
Teacher spread0.214 · 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

Citations6
Published2025
Admission routes1
Has abstractyes

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