activity
20202026
most citedA broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b

145 citations · 387 across the 28 of their papers we have counts for

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Showing 2025Show all

8 papers · 1 filter

astro-ph.EP2025★ 6 cited

Horizontal and vertical exoplanet thermal structure from a JWST spectroscopic eclipse map

Ryan C. Challener, Megan Weiner Mansfield, Patricio E. Cubillos +33

Highly-irradiated giant exoplanets known as "ultra-hot Jupiters" are anticipated to exhibit large variations of atmospheric temperature and chemistry as a function of longitude, la…

astro-ph.EP2025★ 1 cited

Limb Asymmetries on WASP-39b: A Multi-GCM Comparison of Chemistry, Clouds, and Hazes

Maria E. Steinrueck, Arjun B. Savel, Duncan A. Christie +28

With JWST, observing separate spectra of the morning and evening limbs of hot Jupiters has finally become a reality. The first such observation was reported for WASP-39b, where the…

astro-ph.EP2025

A carbon-rich atmosphere on a windy pulsar planet

Michael Zhang, Maya Beleznay, Timothy D. Brandt +17

A handful of enigmatic Jupiter-mass objects have been discovered orbiting pulsars. One such object, PSR\,J2322-2650b, uniquely resembles a hot Jupiter exoplanet due to its minimum…

astro-ph.EP2025★ 7 cited

Strong NUV Refractory Absorption and Dissociated Water in the Hubble Transmission Spectrum of the Ultra Hot Jupiter KELT-20 b

Yayaati Chachan, Joshua Lothringer, Julie Inglis +8

Ultra hot Jupiters (UHJs) present a promising pathway for drawing a link between a planet's composition and formation history. They retain both refractory and volatiles species in…

astro-ph.EP2025

The Roasting Marshmallows Program with IGRINS on Gemini South III: Seeing deeper into the metal depleted atmosphere of a gas-giant on the cusp of the hot to ultra-hot Jupiter transition

Vatsal Panwar, Matteo Brogi, Krishna Kanumalla +17

Ultra-hot Jupiters are a class of gas-giant exoplanets that show a peculiar combination of thermochemical properties in the form of molecular dissociation, atomic ionization, and i…

astro-ph.EP2025

Non-ideal MHD simulations of hot Jupiter atmospheres

Clàudia Soriano-Guerrero, Daniele Viganò, Rosalba Perna +2

In Hot Jupiters (HJs), atmospherically induced magnetic fields are expected to play an important role in controlling the wind circulation and in determining their inflated radii. H…

astro-ph.EP2025

Out on a Limb: The Signatures of East-West Asymmetries in Transmission Spectra from General Circulation Models

Kenneth E. Arnold, Arjun B. Savel, Eliza M. -R. Kempton +5

In the era of JWST, observations of hot Jupiter atmospheres are becoming increasingly precise. As a result, the signature of limb asymmetries due to temperature or abundance differ…

astro-ph.EP2025

The Effects of Kinematic MHD on the Atmospheric Circulation of Eccentric Hot Jupiters

Hayley Beltz, Willow Houck, Laura C. Mayorga +3

Hot Jupiters are typically considered to be tidally locked due to their short orbital periods. The extreme irradiation can result in atmospheric species becoming thermally ionized…