activity
20242026
most citedConstraining the formation of WASP-39b using JWST transit spectroscopy

11 citations · 12 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2026

Energy deposition in planetary and exoplanetary atmospheres induced by cosmic rays

Jesse Polman, Ingo Leya

Cosmic rays can significantly alter the abundances of certain species in the upper layers of planetary atmospheres, especially in terms of their biosignatures. To fully understand…

astro-ph.EP2026

JWST-SUPER I: New insights into irradiated warm Neptunes atmospheres from MIRI observations of HD 106315 c

A. Dyrek, R. Waters, S. -M. Tsai +17

Sulphur-bearing molecules have recently emerged as powerful tracers of atmospheric photochemistry in exoplanets observed with JWST. In several warm giant planets, SO has been d…

astro-ph.EP2026

The formation of planetary systems: physics, populations, and architectures

Andrin Kessler, Jesse Weder, Jesse Polman +5

We review the progresses made in global theoretical models of planetary system formation in the last decade using the example of the planetary system formation framework known as t…

astro-ph.EP2025

Mapping the SO2 Shoreline in Gas Giant Exoplanets

Ian J. M. Crossfield, Eva-Maria Ahrer, Jonathan Brande +8

JWST has revealed sulfur chemistry in giant exoplanet atmospheres, where molecules such as SO2 trace photochemistry, metallicity, and formation and migration. To ascertain the cond…

astro-ph.EP2025★ 1 cited

On Linking Planet Formation Models, Protoplanetary Disk Properties, and Mature Gas Giant Exoplanet Atmospheres

Adina D. Feinstein, Richard A. Booth, Jennifer B. Bergner +34

Measuring a single elemental ratio (e.g., carbon-to-oxygen) provides insufficient information for understanding the formation mechanisms and evolution that affect our observations…

astro-ph.EP2024

Convective mixing in distant and close-in giant planets -- Dependences on the initial composition, luminosity, bloating and semi-convection

Jesse Polman, Christoph Mordasini

Recent structure models of Jupiter suggest the existence of an extended region in the deep interior with a high heavy element abundance, referred to as a dilute core. This finding…

astro-ph.EP2024★ 11 cited

Constraining the formation of WASP-39b using JWST transit spectroscopy

N. Khorshid, M. Min, J. Polman +1

Understanding the formation history of planets is one of the goals of studying exoplanet atmospheres. The atmospheric composition of planets can provide insights into the formation…