activity
20172026
most citedPhotochemical Haze Formation in the Atmospheres of super-Earths and mini-Neptunes

77 citations · 435 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2026★ 1 cited

Elastic Properties of Titan Tholins Revealed by Brillouin Spectroscopy

Mark A. Johnson, Jose R. Montes-Bojorquez, Adis Husic +7

Titan tholins, complex organic solids synthesized by simulating photochemical processes in Titan's atmosphere, are widely regarded as analogs to organic surface materials on the Sa…

astro-ph.EP2026

A Cross-Laboratory Comparison Study of Titan Haze Analogs: Surface Energy II

Eric C. Austin, Xinting Yu, Chao He +10

The organic haze particles on Titan play important roles in atmospheric cloud formation and aerosol-lake interactions. These processes are strongly influenced by the surface energy…

astro-ph.EP2024

Probing Cold-to-Temperate Exoplanetary Atmospheres: The Role of Water Condensation on Surface Identification with JWST

Ziyu Huang, Xinting Yu, Shang-Min Tsai +5

Understanding the surface temperature and interior structure of cold-to-temperate sub-Neptunes is critical for assessing their habitability, yet direct observations are challenging…

astro-ph.EP2024★ 14 cited

The Fate of Simple Organics on Titan's Surface: A Theoretical Perspective

Xinting Yu, Yue Yu, Julia Garver +2

Atmospheric photochemistry on Titan continuously transforms methane and nitrogen gases into various organic compounds. This study explores the fate of these molecules when they lan…

astro-ph.EP2022★ 18 cited

Material Properties of Organic Liquids, Ices, and Hazes on Titan

Xinting Yu, Yue Yu, Julia Garver +5

Titan has a diverse range of materials in its atmosphere and on its surface: the simple organics that reside in various phases (gas, liquid, ice) and the solid complex refractory o…

astro-ph.EP2022★ 19 cited

Microphysics of Water Clouds in the Atmospheres of Y Dwarfs and Temperate Giant Planets

James Mang, Peter Gao, Callie E. Hood +4

Water clouds are expected to form on Y dwarfs and giant planets with equilibrium temperatures near or below that of Earth, drastically altering their atmospheric compositions and t…