MétaCan
Menu
← Back to cohort
Record W4311000394 · doi:10.1093/mnras/stac3639

Discovery of TOI-1260d and the characterization of the multiplanet system

2022· article· en· W4311000394 on OpenAlexfundno aff
K. W. F. Lam, J. Cabrera, M. J. Hooton, Y. Alibert, A. Bonfanti, M. Beck, A. Deline, H-G Florén, A. E. Simon, L. Fossati, C. M. Persson, M. Fridlund, Sébastien Salmon, S. Hoyer, H. P. Osborn, T. G. Wilson, Iskra Georgieva, Gr Nowak, R. Luque, J. A. Egger, V. Adibekyan, R. Alonso, G. Anglada‐Escudé, T. Bárczy, D. Barrado, S. C. C. Barros, W. Baumjohann, T. Beck, A. Bekkelien, W. Benz, N. Billot, X. Bonfıls, A. Brandeker, C. Broeg, S. Charnoz, A. Collier Cameron, Sz. Csizmadia, M. B. Davies, M. Deleuil, L. Delrez, O. D. S. Demangeon, D. Ehrenreich, A. Erikson, A. Fortier, D. Futyan, D. Gandolfi, M. Gillon, M. Guêdel, P. Guterman, J. Laskar, David W. Latham, A. Lecavelier des Étangs, M. Lendl, C. Lovis, Kevin Heng, K. G. Isaak, L. L. Kiss, Demetrio Magrin, P. F. L. Maxted, V. Nascimbeni, G. Olofsson, R. Ottensamer, I. Pagano, Ε. Πάλλη, G. Peter, G. Piotto, D. Pollacco, D. Queloz, I. Ribas, Roberto Ragazzoni, N. Rando, H. Rauer, N. C. Santos, G. Scandariato, Sara Seager, D. Ségransan, L. M. Serrano, A. M. S. Smith, S. G. Sousa, M. Steller, Gy. M. Szabó, N. Thomas, S. Udry, V. Van Grootel, N. A. Walton, Joshua N. Winn

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersH2020 European Research CouncilNuclear Fuel Cycle and Supply ChainEuropean Regional Development FundScience and Technology Facilities CouncilInstitut sur la Nutrition et les Aliments FonctionnelsNemzeti Kutatási Fejlesztési és Innovációs HivatalGeneralitat de CatalunyaFederación Española de Enfermedades RarasFundação para a Ciência e a TecnologiaCentre National d’Etudes SpatialesEntomological Society of AmericaFonds De La Recherche Scientifique - FNRSUniversidad de La LagunaSwedish National Space AgencyNational Research, Development and Innovation OfficeSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungEötvös Loránd TudományegyetemUniversité de LiègeFondazione CRTEuropean CommissionMinisterio de Ciencia e InnovaciónNational Science FoundationBelgian Federal Science Policy OfficeDeutsche ForschungsgemeinschaftCentres de Recerca de CatalunyaNational Aeronautics and Space AdministrationAgenzia Spaziale ItalianaEuropean Space AgencyAgence Nationale de la RechercheSpace Telescope Science InstituteUK Space Agency
KeywordsPhysicsPlanetPhotometry (optics)AstrophysicsRADIUSNeptuneAstronomyOrbital periodPlanetary systemEarth radiusStars

Abstract

fetched live from OpenAlex

ABSTRACT We report the discovery of a third planet transiting the star TOI-1260, previously known to host two transiting sub-Neptune planets with orbital periods of 3.127 and 7.493 d, respectively. The nature of the third transiting planet with a 16.6-d orbit is supported by ground-based follow-up observations, including time-series photometry, high-angular resolution images, spectroscopy, and archival imagery. Precise photometric monitoring with CHEOPS allows to improve the constraints on the parameters of the system, improving our knowledge on their composition. The improved radii of TOI-1260b and TOI-1260c are $2.36 \pm 0.06 \rm R_{\oplus }$, $2.82 \pm 0.08 \rm R_{\oplus }$, respectively while the newly discovered third planet has a radius of $3.09 \pm 0.09 \rm R_{\oplus }$. The radius uncertainties are in the range of 3 per cent, allowing a precise interpretation of the interior structure of the three planets. Our planet interior composition model suggests that all three planets in the TOI-1260 system contains some fraction of gas. The innermost planet TOI-1260b has most likely lost all of its primordial hydrogen-dominated envelope. Planets c and d were also likely to have experienced significant loss of atmospheric through escape, but to a lesser extent compared to planet b.

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.006

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 communication0.0010.000
Open science0.0000.001
Research integrity0.0010.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.171
Teacher spread0.166 · 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

Citations8
Published2022
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicStellar, planetary, and galactic studies→French-language works237,207→