activity
20242026
most citedImpacts of Atmospheric Carbon Species and Stellar Type on Climates of Terrestrial Planets

1 citations · 1 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2026

Tempawral: A Time-Resolved Retrieval Framework for Variable Brown Dwarfs and Exoplanets

Fei Wang, Ben Burningham, Stuart Littlefair +4

Brown dwarfs and exoplanets are thought to host complex atmospheric phenomena such as clouds, storms, and chemical heterogeneity, akin to weather patterns on Earth. These features…

astro-ph.EP2026

Probing thermal gradients of habitable-zone rocky planets as an anti-indicator of a global surface ocean using mid-infrared direct imaging

Yuka Fujii, Daniel Angerhausen, Taro Matsuo +1

Future direct-imaging missions such as the Large Interferometer for Exoplanets (LIFE) aim to observe thermal emission from potentially habitable planets to characterize their surfa…

astro-ph.IM2025

On the synergetic use of Ariel and JWST for exoplanet atmospheric science

Quentin Changeat, Pierre-Olivier Lagage, Giovanna Tinetti +27

This paper explores the potential for strategic synergies between the JWST and the Ariel telescopes, two flagship observatories poised to revolutionise the study of exoplanet atmos…

astro-ph.EP20251 cited

Impacts of Atmospheric Carbon Species and Stellar Type on Climates of Terrestrial Planets

Jared Landry, Hiroyuki Kurokawa, Tetsuo Taki +3

The climates of terrestrial planets are largely determined by the composition of their atmospheres and spectral types of their host stars. Previous studies suggest a wide range of…

astro-ph.EP2025

Monosilane Worlds: Sub-Neptunes with Atmospheres Shaped by Reduced Magma Oceans

Yuichi Ito, Tadahiro Kimura, Kazumasa Ohno +2

High-precision infrared spectroscopic measurements now enable detailed characterization of sub-Neptune atmospheres, potentially providing constraints on their interiors. Motivated…

astro-ph.EP2024

Role of magma oceans in controlling carbon and oxygen of sub-Neptune atmospheres

Chanoul Seo, Yuichi Ito, Yuka Fujii

Most exoplanets with a few Earth radii are more inflated than bare-rock planets with the same mass, indicating a substantial volatile amount. Neither the origin of the volatiles no…