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Record W4310618280 · doi:10.17615/yy9t-h782

TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full-frame Images

2022· article· en· W4310618280 on OpenAlexfundno aff
D.J. Wright, J. Kielkopf, A. Jordán, S.R. Kane, R.A. Matson, E.W. Guenther, N. Grieves, M.L. Calkins, S. Cartwright, G. Chaverot, D.J. Stevens, C. Stibbards, R.G. West, K. Eastridge, R.A. Wittenmyer, J.E. Rodriguez, R. Brahm, E.L.N. Jensen, D.J. James, A. E. Granados, N. Guerrero, L. Gordon, C.E. Henze, T. Henning, M. Esposito, David R. Ciardi, C.X. Huang, K.I. Collins, Peter Plavchan, J.L. Christiansen, Parker Reed, K. Hesse, B. Skinner, David Baker, Gavin Wang, R.J. Siverd, C.G. Tinney, N. Latouf, L.D. Nielsen, R.B. Kuhn, S. Vach, George Zhou, J. D. Eastman, C. Hellier, R.J. Oelkers, J. Wittrock, T.-G. Tan, P. Berlind, B. Addison, S.N. Quinn, T.G. Beatty, A. Bieryla, J.M. Jenkins, K.A. Collins, A.M. Levine, K. Kim, J. N. Winn, Andrew W. Mann, S. Mao, H. Zhang, D.A. Caldwell, D.L. Feliz, M. Stalport, P. Chaturvedi, G.A. Esquerdo, T. Barclay, S. Chimaladinne, N. Espinoza, I.J.M. Crossfield, D.R. Anderson, D.A. Yahalomi, A. Vanderburg, B.S. Gaudi, S. Christian, K.G. Stassun, R.P. Schwarz, D. J. Radford, M. Bowen, F. Bouchy, Mario Santiago Jiménez, E. Matthews, E. J. Gonzales, G.R. Ricker, J. Okumura, M.W. Mengel, J. Mink, J. Pepper, T. O apos Dwyer, A.B. Savel, E. Palle, P. Newman, P. Sarkis, E.V. Quintana, K.K. McLeod, B.P. Bowler, Mélissa J. Hobson, R.K. Vanderspek, David W. Latham, I. Carleo, C.D. Dressing, S. Seager, C. Ziegler, T. Gan, C.E. Brasseur, C. Briceño, N.M. Law, J. Horner, J. V. Seidel, R. Sefako, C. Schnaible, S.B. Howell, A. Shporer, J.E. Schlieder, W. Fong, M.B. Lund, S. Giacalone, H. Gill, Tyler Fenske

Bibliographic record

VenueUNC Libraries · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstronomy and Astrophysical Research
Canadian institutionsnot available
FundersScience Mission DirectorateCollege of Engineering, Michigan State UniversityNuclear Safety and Security CommissionUniversity of North Carolina at Chapel HillEuropean CommissionCorporación de Fomento de la ProducciónPennsylvania State UniversityUniversity of TorontoMichigan State UniversityPennsylvania Space Grant ConsortiumOhio State UniversityDeutsche ForschungsgemeinschaftFund for Astrophysical ResearchNational Science FoundationEuropean Space AgencyMinistério da Ciência, Tecnologia e InovaçãoNational Aeronautics and Space Administration
KeywordsPlanetStarsFrame (networking)AstronomyAstrobiologyPhysicsAstrophysicsComputer scienceTelecommunications

Abstract

fetched live from OpenAlex

We present the discovery and characterization of five hot and warm Jupiters - TOI-628 b (TIC 281408474; HD 288842), TOI-640 b (TIC 147977348), TOI-1333 b (TIC 395171208, BD+47 3521A), TOI-1478 b (TIC 409794137), and TOI-1601 b (TIC 139375960) - based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The five planets were identified from the full-frame images and were confirmed through a series of photometric and spectroscopic follow-up observations by the TESS Follow-up Observing Program Working Group. The planets are all Jovian size (R P = 1.01-1.77 R J) and have masses that range from 0.85 to 6.33 M J. The host stars of these systems have F and G spectral types (5595 ≤ T eff ≤ 6460 K) and are all relatively bright (9.5 < V < 10.8, 8.2 < K < 9.3), making them well suited for future detailed characterization efforts. Three of the systems in our sample (TOI-640 b, TOI-1333 b, and TOI-1601 b) orbit subgiant host stars (log g < 4.1). TOI-640 b is one of only three known hot Jupiters to have a highly inflated radius (R P > 1.7 R J, possibly a result of its host star's evolution) and resides on an orbit with a period longer than 5 days. TOI-628 b is the most massive, hot Jupiter discovered to date by TESS with a measured mass of 6.31-0.30+0.28 M J and a statistically significant, nonzero orbital eccentricity of e = 0.074-0.022+0.021. This planet would not have had enough time to circularize through tidal forces from our analysis, suggesting that it might be remnant eccentricity from its migration. The longest-period planet in this sample, TOI-1478 b (P = 10.18 days), is a warm Jupiter in a circular orbit around a near-solar analog. NASA's TESS mission is continuing to increase the sample of well-characterized hot and warm Jupiters, complementing its primary mission goals.

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 categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.293
Threshold uncertainty score0.994

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0010.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0070.000

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 head0.011
GPT teacher head0.214
Teacher spread0.204 · 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 designTheoretical or conceptual
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
Published2022
Admission routes1
Has abstractyes

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