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Record W3121294479

Near-resonance in a System of Sub-Neptunes from <i>TESS</i>

2019· article· en· W3121294479 on OpenAlexaff
Samuel N. Quinn, Juliette Becker, Joseph E. Rodriguez, Sam Hadden, Chelsea X. Huang, Timothy D. Morton, Fred C. Adams, D. J. Armstrong, Jason D. Eastman, Jonathan Horner, Stephen R. Kane, Jack J. Lissauer, Joseph D. Twicken, Andrew Vanderburg, Rob Wittenmyer, G. Ricker, R. Vanderspek, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins, Eric Agol, Khalid Barkaoui, Charles Beichman, F. Bouchy, Luke G. Bouma, Artem Burdanov, J. Campbell, Roberto Carlino, Scott Cartwright, David Charbonneau, Jessie L. Christiansen, David R. Ciardi, Karen A. Collins, Kevin I. Collins, Dennis M. Conti, Ian J. M. Crossfield, Tansu Daylan, Jason Dittmann, J. Doty, Diana Dragomir, Elsa Ducrot, M. Gillon, Ana Glidden, Robert F. Goeke, Erica J. Gonzales, K. G. Hełminiak, Elliott P. Horch, Steve B. Howell, Emmanuël Jehin, Eric L. N. Jensen, John F. Kielkopf, Martti H. Kristiansen, Nicholas M. Law, Andrew W. Mann, M. Marmier, Rachel A. Matson, Elisabeth C. Matthews, T. Mazeh, M. Mori, F. Murgas, C. A. Murray, Norio Narita, Louise D. Nielsen, G. Ottoni, Ε. Πάλλη, R. Pawłaszek, F. Pepe, Jerome Pitogo de Leon, F. J. Pozuelos, Howard M. Relles, Joshua E. Schlieder, Daniel Sebastian, D. Ségransan, Avi Shporer, Keivan G. Stassun, Motohide Tamura, S. Udry, Ian Waite, Jennifer G. Winters, Carl Ziegler

Bibliographic record

VenueUniversity of Southern Queensland ePrints (University of Southern Queensland) · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
Fundersnot available
KeywordsPhysicsResonance (particle physics)AstronomyPlanetary systemAstrophysicsAstrobiologyStarsParticle physics
DOInot available

Abstract

fetched live from OpenAlex

We report the Transiting Exoplanet Survey Satellite detection of a multi-planet system orbiting the V = 10.9 K0 dwarf TOI-125. We find evidence for up to five planets, with varying confidence. Three transit signals with high signal-to-noise ratio correspond to sub-Neptune-sized planets (2.76, 2.79, and 2.94 R <SUB>⊕</SUB>), and we statistically validate the planetary nature of the two inner planets (P <SUB> b </SUB> = 4.65 days, P <SUB> c </SUB> = 9.15 days). With only two transits observed, we report the outer object (P <SUB>.03</SUB> = 19.98 days) as a planet candidate with high signal-to-noise ratio. We also detect a candidate transiting super-Earth (1.4 R <SUB>⊕</SUB>) with an orbital period of only 12.7 hr and a candidate Neptune-sized planet (4.2 R <SUB>⊕</SUB>) with a period of 13.28 days, both at low signal-to-noise ratio. This system is amenable to mass determination via radial velocities and transit-timing variations, and provides an opportunity to study planets of similar size while controlling for age and environment. The ratio of orbital periods between TOI-125 b and c (P <SUB> c </SUB>/P <SUB> b </SUB> = 1.97) is slightly lower than an exact 2:1 commensurability and is atypical of multiple planet systems from Kepler, which show a preference for period ratios just wide of first-order period ratios. A dynamical analysis refines the allowed parameter space through stability arguments and suggests that despite the nearly commensurate periods, the system is unlikely to be in resonance.

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 categoriesMeta-epidemiology (narrow), Insufficient payload (model declined to judge)
Consensus categoriesInsufficient payload (model declined to judge)
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.218
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.000
Science and technology studies0.0000.001
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.001

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 head0.151
Teacher spread0.146 · 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; both teacher heads agree on what is shown here.

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

Citations46
Published2019
Admission routes1
Has abstractyes

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