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20242026
most citedJWST/NIRISS reveals the water-rich "steam world" atmosphere of GJ 9827 d

92 citations · 273 across the 28 of their papers we have counts for

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astro-ph.EP2024★ 92 cited

JWST/NIRISS reveals the water-rich "steam world" atmosphere of GJ 9827 d

Caroline Piaulet-Ghorayeb, Bjorn Benneke, Michael Radica +30

With sizable volatile envelopes but smaller radii than the solar system ice giants, sub-Neptunes have been revealed as one of the most common types of planet in the galaxy. While t…

astro-ph.EP2024★ 23 cited

BOWIE-ALIGN: JWST reveals hints of planetesimal accretion and complex sulphur chemistry in the atmosphere of the misaligned hot Jupiter WASP-15b

James Kirk, Eva-Maria Ahrer, Alastair B. Claringbold +23

We present a transmission spectrum of the misaligned hot Jupiter WASP-15b from 2.8-5.2 microns observed with JWST's NIRSpec/G395H grating. Our high signal to noise data, which has…

astro-ph.EP2024

Inhomogeneous terminators on the exoplanet WASP-39 b

Néstor Espinoza, Maria E. Steinrueck, James Kirk +40

Transmission spectroscopy has been a workhorse technique over the past two decades to constrain the physical and chemical properties of exoplanet atmospheres. One of its classical…

astro-ph.EP2024★ 32 cited

BOWIE-ALIGN: How formation and migration histories of giant planets impact atmospheric compositions

Anna B. T. Penzlin, Richard A. Booth, James Kirk +15

Hot Jupiters present a unique opportunity for measuring how planet formation history shapes present-day atmospheric composition. However, due to the myriad pathways influencing com…

astro-ph.EP2024★ 16 cited

BOWIE-ALIGN: A JWST comparative survey of aligned vs misaligned hot Jupiters to test the dependence of atmospheric composition on migration history

James Kirk, Eva-Maria Ahrer, Anna B. T. Penzlin +19

A primary objective of exoplanet atmosphere characterisation is to learn about planet formation and evolution, however, this is challenged by degeneracies. To determine whether dif…

astro-ph.EP2024★ 1 cited

The CUISINES Framework for Conducting Exoplanet Model Intercomparison Projects, Version 1.0

Linda E. Sohl, Thomas J. Fauchez, Shawn Domagal-Goldman +10

As JWST begins to return observations, it is more important than ever that exoplanet climate models can consistently and correctly predict the observability of exoplanets, retrieva…

astro-ph.EP2024

Longitudinal Filtering, Sponge Layers, and Equatorial Jet Formation in a General Circulation Model of Gaseous Exoplanets

D. A. Christie, N. J. Mayne, M. Zamyatina +4

General circulation models are a useful tool in understanding the three dimensional structure of hot Jupiter and sub-Neptune atmospheres; however, understanding the validity of the…

astro-ph.EP2024★ 29 cited

JWST Reveals CH, CO, and HO in a Metal-rich Miscible Atmosphere on a Two-Earth-Radius Exoplanet

Björn Benneke, Pierre-Alexis Roy, Louis-Philippe Coulombe +28

Even though sub-Neptunes likely represent the most common outcome of planet formation, their natures remain poorly understood. In particular, planets near 1.5-2.5 often…

astro-ph.EP2024★ 1 cited

Quenching-driven equatorial depletion and limb asymmetries in hot Jupiter atmospheres: WASP-96b example

Maria Zamyatina, Duncan A. Christie, Eric Hébrard +11

Transport-induced quenching in hot Jupiter atmospheres is a process that determines the boundary between the part of the atmosphere at chemical equilibrium and the part of the atmo…