MétaCan
Menu
← Back to cohort
Record W3196101103 · doi:10.3847/1538-3881/ac1ba3

TOI-1518b: A Misaligned Ultra-hot Jupiter with Iron in Its Atmosphere

2021· preprint· en· W3196101103 on OpenAlexaff
Samuel H. C. Cabot, Aaron Bello-Arufe, João M. Mendonça, R. Tronsgaard, Ian Wong, George Zhou, Lars A. Buchhave, Debra A. Fischer, Keivan G. Stassun, V. Antoci, David Baker, A. Belinski, Björn Benneke, Luke G. Bouma, Jessie L. Christiansen, Karen A. Collins, Maria V. Goliguzova, Simone R. Hagey, Jon M. Jenkins, Eric L. N. Jensen, Richard C. Kidwell, Didier Laloum, Bob Massey, Kim K. McLeod, David W. Latham, E. Morgan, G. Ricker, Boris S. Safonov, Joshua E. Schlieder, Sara Seager, Avi Shporer, Jeffrey C. Smith, Gregor Srdoč, Ivan A. Strakhov, Guillermo Torres, Joseph D. Twicken, R. Vanderspek, Michael Vezie, Joshua N. Winn

Bibliographic record

VenueThe Astronomical Journal · 2021
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversity of SaskatchewanUniversité de Montréal
FundersLomonosov Moscow State UniversityNew York Community TrustFund for Astrophysical ResearchStellar Astrophysics CentreNational Research FoundationAmes Research CenterMinistry of Science and Higher Education of the Russian FederationNational Science FoundationYale UniversityDanmarks GrundforskningsfondNational Aeronautics and Space AdministrationVillum Fonden
KeywordsPhysicsAstrophysicsHot JupiterPlanetJupiter (rocket family)Atmosphere (unit)OccultationFlux (metallurgy)Brightness temperatureBrightnessAstronomyExoplanetChemistry

Abstract

fetched live from OpenAlex

Abstract We present the discovery of TOI-1518b—an ultra-hot Jupiter orbiting a bright star (V = 8.95). The transiting planet is confirmed using high-resolution optical transmission spectra from EXPRES. It is inflated, with R p = 1.875 ± 0.053 R J, and exhibits several interesting properties, including a misaligned orbit ( 240.34 − 0.98 + 0.93 degrees) and nearly grazing transit ( b = 0.9036 − 0.0053 + 0.0061 ). The planet orbits a fast-rotating F0 host star (T eff ≃ 7300 K) in 1.9 days and experiences intense irradiation. Notably, the TESS data show a clear secondary eclipse with a depth of 364 ± 28 ppm and a significant phase-curve signal, from which we obtain a relative day–night planetary flux difference of roughly 320 ppm and a 5.2σ detection of ellipsoidal distortion on the host star. Prompted by recent detections of atomic and ionized species in ultra-hot Jupiter atmospheres, we conduct an atmospheric cross-correlation analysis. We detect neutral iron (5.2σ), at K p = 157 − 44 + 68 km s−1 and V sys = − 16 − 4 + 2 , adding another object to the small sample of highly irradiated gas-giant planets with Fe detections in transmission. Detections so far favor particularly inflated gas giants with radii ≳1.78 R J, which may be due to observational bias. With an equilibrium temperature of T eq = 2492 ± 38 K and a measured dayside brightness temperature of 3237 ± 59 K (assuming zero geometric albedo), TOI-1518b is a promising candidate for future emission spectroscopy to probe for a thermal inversion.

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 score0.002
Threshold uncertainty score0.005

Distilled classifier scores by category (both heads)

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 science0.0000.000
Research integrity0.0010.000
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 head0.011
GPT teacher head0.221
Teacher spread0.210 · 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

Citations0
Published2021
Admission routes1
Has abstractyes

Explore more

Same venueThe Astronomical Journal→Same topicStellar, planetary, and galactic studies→French-language works237,207→