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Record W4310620191 · doi:10.17615/19kp-3d84

HD 2685 b: A hot Jupiter orbiting an early F-type star detected by TESS

2022· article· en· W4310620191 on OpenAlexfundno aff
D. Ségransan, F. Pepe, D. Osip, J. Doty, E. Sedaghati, H. Relles, C. Ziegler, P. Tenenbaum, J.M. Jenkins, L. D. Nielsen, B. Cruz, L.A. Paredes, P. Sarkis, E. Matthews, G. Furész, D. Bayliss, T. Henning, C. Lovis, K. Haworth, R. Matson, J. Schlieder, O. Turner, A. Vanderburg, N.M. Law, Rafael Brahm, M.I. Jones, G. Á. Bakos, S. Howell, David W. Latham, A. Jordán, J. Dittmann, Jessie L. Christiansen, A.W. Mann, E. Gonzales, T. Henry, J. Hodari-Sadiki, V. Suc, J.N. Winn, M. Marmier, A. Tokovinin, S. Udry, M. Davies, J.C. Smith, F. Bouchy, I. Crossfield, S. Seager, G. Laughlin, K. A. Collins, Avi Shporer, S. Wang, N. Espinoza, C. Beichman, D. Ciardi

Bibliographic record

VenueMPG.PuRe (Max Planck Society) · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsnot available
FundersComisión Nacional de Investigación Científica y TecnológicaNASA Exoplanet Science InstituteNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyJet Propulsion LaboratoryUniversity of Toronto
KeywordsStar (game theory)Jupiter (rocket family)AstronomyPhysicsAstrophysicsAstrobiologySpacecraft

Abstract

fetched live from OpenAlex

We report on the confirmation of a transiting giant planet around the relatively hot (Teff = 6801 ± 76 K) star HD 2685, whose transit signal was detected in Sector 1 data of NASA's TESS mission. We confirmed the planetary nature of the transit signal using Doppler velocimetric measurements with CHIRON, CORALIE, and FEROS, as well as using photometric data obtained with the Chilean-Hungarian Automated Telescope and the Las Cumbres Observatory. From the joint analysis of photometry and radial velocities, we derived the following parameters for HD 2685 b: P = 4.12688-0.00004+0.00005 days, e = 0.091-0.047+0.039, MP = 1.17 ± 0.12 MJ, and RP =1.44 ± 0.05 RJ. This system is a typical example of an inflated transiting hot Jupiter in a low-eccentricity orbit. Based on the apparent visual magnitude (V = 9.6 mag) of the host star, this is one of the brightest known stars hosting a transiting hot Jupiter, and it is a good example of the upcoming systems that will be detected by TESS during the two-year primary mission. This is also an excellent target for future ground- and space-based atmospheric characterization as well as a good candidate for measuring the projected spin-orbit misalignment angle through the Rossiter-McLaughlin effect.

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.452
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0030.000

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 head0.008
GPT teacher head0.200
Teacher spread0.192 · 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

Citations0
Published2022
Admission routes1
Has abstractyes

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