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Record W4416685571 · doi:10.1051/0004-6361/202556257

Atmospheric composition and circulation of the ultra-hot Jupiter WASP-121b with joint NIRPS, HARPS and CRIRES+ transit spectroscopy

2025· article· en· W4416685571 on OpenAlexaff
Valentina Vaulato, Mélissa J. Hobson, Romain Allart, Stefan Pelletier, Joost P. Wardenier, H. Chakraborty, D. Ehrenreich, N. Nari, M. Steiner, X. Dumusque, H. J. Hoeijmakers, Étienne Artigau, Frédérique Baron, S. C. C. Barros, Björn Benneke, X. Bonfıls, F. Bouchy, Marta L. Bryan, B. L. Canto Martins, Ryan Cloutier, Neil J. Cook, Nicolas B. Cowan, J. R. De Medeiros, X. Delfosse, E. Delgado Mena, René Doyon, J. I. Gónzalez Hernández, David Lafreniére, I. C. Leão, C. Lovis, Lison Malo, C. Melo, L. Mignon, C. Mordasini, F. Pepe, R. Rébolo, Jason F. Rowe, N. C. Santos, D. Ségransan, A. Suárez Mascareño, S. Udry, Diana Valencia, G. A. Wade, J. G. De S. Aguiar, Khaled Al Moulla, B. Akinsanmi, Nicholas W. Borsato, Charles Cadieux, Yann Carteret, Ana Rita Costa Silva, E. Cristo, T. Forveille, Yolanda G. C. Frensch, Nicole Gromek, M. Lendl, Bibiana Prinoth, Angelica Psaridi, Atanas K. Stefanov, B. Thorsbro, Drew Weisserman

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsMcGill UniversityQueen's UniversityMcMaster UniversityRoyal Military College of CanadaUniversity of TorontoUniversité de MontréalMontreal Clinical Research Institute
Fundersnot available
KeywordsRadial velocityTransit (satellite)PlanetHot JupiterAtmospheric chemistrySpectroscopyAtmospheric modelsAtmospheric modelAtmosphere (unit)

Abstract

fetched live from OpenAlex

Ultra-hot gas giants such as WASP-121b provide unique laboratories for exploring atmospheric chemistry and dynamics under extreme irradiation conditions. Uncovering their chemical composition and atmospheric circulation is critical for tracing planet formation pathways. Here, we present a comprehensive atmospheric characterisation of WASP-121b using high-resolution transit spectroscopy across the optical to infrared with HARPS, NIRPS, and CRIRES+ spanning nine transit events. These observations are complemented with five TESS photometric sectors, two EulerCam light curves simultaneous to the HARPS and NIRPS transits, and an extensive radial velocity dataset in order to refine WASP-121b's orbital parameters. A cross-correlation analysis detected iron (Fe), carbon monoxide (CO) and vanadium (V) absorption signals with SNR of 5.8, 5.0, and 4.7, respectively. Our retrieval analysis constrains the water (H 2 O) abundance to −6.52 −0.68 +0.49 dex, although its absorption signal is effectively muted by the hydride (H − ) continuum. We constrained the relative abundances of the volatile and refractory elements - which represents a crucial diagnostic of atmospheric chemistry, evolution, and planet formation pathways. The retrieved abundance ratios are broadly consistent with expected values of a solar composition atmosphere in chemical equilibrium, likely indicating minimal disequilibrium chemistry alterations at the probed pressures (∼10 −4 −10 −3 bar). We update the orbital parameters of WASP-121b with its largest radial velocity dataset to date. By comparing orbital velocities derived from both the radial velocity analysis and the atmospheric retrieval, we determined a non-zero velocity offset caused by atmospheric circulation, ΔK p = −15 ± 3 km s −1 (assuming M ⋆ = 1.38 ± 0.02 M ⊙ ), consistent with predictions from either drag-free or weak-drag 3D global circulation models, while we caution the non-negligible dependence on the assumed stellar mass. These results place new constraints on the thermal structure, dynamics, and chemical inventory of WASP-121b, highlighting the power of multi-wavelength high-resolution spectroscopy to probe exoplanetary atmospheres.

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: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.011
Threshold uncertainty score0.023

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0000.001
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 head0.005
GPT teacher head0.184
Teacher spread0.180 · 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

Citations1
Published2025
Admission routes1
Has abstractyes

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