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Record W3099767647

TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite

2020· article· en· W3099767647 on OpenAlexaff
Rafael Brahm, Louise D. Nielsen, Robert A. Wittenmyer, Songhu Wang, Joseph E. Rodriguez, Néstor Espinoza, M. I. Jones, Andrés Jordán, Thomas Henning, Mélissa J. Hobson, D. Kossakowski, Felipe Rojas, P. Sarkis, Martin Schlecker, Trifon Trifonov, S. Shahaf, G. Ricker, R. Vanderspek, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins, Brett Addison, G. Á. Bakos, W. Bhatti, Daniel Bayliss, P. Berlind, Allyson Bieryla, F. Bouchy, Brendan P. Bowler, César Briceño, Timothy M. Brown, Edward M. Bryant, Douglas A. Caldwell, David Charbonneau, Karen A. Collins, Allen B. Davis, Gilbert A. Esquerdo, Benjamin J. Fulton, Natalia Guerrero, Christopher E. Henze, Aleisha Hogan, Jonathan Horner, Chelsea X. Huang, Jonathan Irwin, Stephen R. Kane, John F. Kielkopf, Andrew W. Mann, T. Mazeh, J. McCormac, C. McCully, Matthew W. Mengel, Ismael Mireles, Jack Okumura, Peter Plavchan, Samuel N. Quinn, M. Rabus, S. Saesen, Joshua E. Schlieder, D. Ségransan, Bernie Shiao, Avi Shporer, Robert J. Siverd, Keivan G. Stassun, V. Suc, P. Torres, C. G. Tinney, S. Udry, L. Vanzi, Michael Vezie, José I Vines, M. Vučković, D. J. Wright, Daniel A. Yahalomi, A. Zapata, Hui Zhang, Carl Ziegler

Bibliographic record

VenueUniversity of Southern Queensland ePrints (University of Southern Queensland) · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
Fundersnot available
KeywordsPhysicsExoplanetStar (game theory)Hot JupiterAstrophysicsOrbital periodRADIUSPlanetType (biology)Gas giantStarsBiology
DOInot available

Abstract

fetched live from OpenAlex

We present the discovery of two new 10 day period giant planets from the Transiting Exoplanet Survey Satellite mission, whose masses were precisely determined using a wide diversity of ground-based facilities. TOI-481 b and TOI-892 b have similar radii (0.99 ± 0.01 ${R}_{{\\rm{J}}}$ and 1.07 ± 0.02 ${R}_{{\\rm{J}}}$, respectively), and orbital periods (10.3311 days and 10.6266 days, respectively), but significantly different masses (1.53 ± 0.03 ${M}_{{\\rm{J}}}$ versus 0.95 ± 0.07 ${M}_{{\\rm{J}}}$, respectively). Both planets orbit metal-rich stars ($[\\mathrm{Fe}/{\\rm{H}}]$ = $+0.26\\pm 0.05$ dex and $[\\mathrm{Fe}/{\\rm{H}}]$ = $+0.24\\pm 0.05$ for TOI-481 and TOI-892, respectively) but at different evolutionary stages. TOI-481 is a ${M}_{\\star }$ = 1.14 ± 0.02 ${M}_{\\odot }$, ${R}_{\\star }$ = 1.66 ± 0.02 ${R}_{\\odot }$ G-type star (${T}_{\\mathrm{eff}}$ = $5735\\pm 72$ K), that with an age of 6.7 Gyr, is in the turn-off point of the main sequence. TOI-892 on the other hand, is a F-type dwarf star (${T}_{\\mathrm{eff}}$ = $6261\\pm 80$ K), which has a mass of ${M}_{\\star }$ = 1.28 ± 0.03 ${M}_{\\odot }$ and a radius of ${R}_{\\star }$ = 1.39 ± 0.02 ${R}_{\\odot }$. TOI-481 b and TOI-892 b join the scarcely populated region of transiting gas giants with orbital periods longer than 10 days, which is important to constrain theories of the formation and structure of hot Jupiters.

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 categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.081
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 studies0.0010.001
Scholarly communication0.0000.000
Open science0.0010.000
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 head0.016
GPT teacher head0.179
Teacher spread0.162 · 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 teacher head, not a consensus.

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

Citations33
Published2020
Admission routes1
Has abstractyes

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