collaborators

10 papers

astro-ph.EP2026

JWST Transmission Spectroscopy of TOI-3235 b: Challenges in Constraining Giant Planet Atmospheres Around M Dwarfs Amid Stellar Contamination

Zoe Ko, Néstor Espinoza, Andrés Jordán +7

Giant planets orbiting low-mass M dwarfs challenge current planet formation theories, which predict that such planets are unlikely to form. Characterizing their atmospheres can pro…

astro-ph.EP2026

The Role of Formation Location in Shaping Sulfur-, Nitrogen-, and Carbon-Bearing Species in Super-Earth and Sub-Neptune Atmospheres

Aaron Werlen, Remo Burn, Caroline Dorn +2

Atmospheric compositions of sub-Neptunes and super-Earths are often interpreted as tracers of formation location relative to volatile ice lines. However, prolonged magma oceans can…

astro-ph.EP2025

Exoplanet formation inference using conditional invertible neural networks

Remo Burn, Victor F. Ksoll, Hubert Klahr +1

The interpretation of the origin of observed exoplanets is usually done only qualitatively due to uncertainties of key parameters in planet formation models. To allow a quantitativ…

astro-ph.EP2025

Water-rich sub-Neptunes and rocky super Earths around different Stars: Radii shaped by Volatile Partitioning, Formation, and Evolution

Remo Burn, Komal Bali, Caroline Dorn +2

The nature of sub-Neptunes remains unknown due to degeneracies in interior structure solutions. However, a statistical set of small planets with measured masses and radii can be us…

astro-ph.EP2025

The New Generation Planetary Population Synthesis (NGPPS). VII. Statistical comparison with the HARPS/Coralie survey

Alexandre Emsenhuber, Christoph Mordasini, Michel Mayor +8

We seek to quantify the fidelity with which modern population syntheses reproduce observations in view of their use as predictive tools. We compared synthetic populations from the…

astro-ph.EP2025

Sub-Neptunes Are Drier Than They Seem: Rethinking the Origins of Water-Rich Worlds

Aaron Werlen, Caroline Dorn, Remo Burn +3

Recent claims of biosignature gases in sub-Neptune atmospheres have renewed interest in water-rich sub-Neptunes with surface oceans, often referred to as Hycean planets. These plan…