Observations of substellar atmospheres

I leverage state-of-the-art observational data from telescopes such as HST and JWST to characterize the atmospheres of exoplanets and brown dwarfs. My work focuses on interpreting transmission and emission spectra to detect key chemical species and cloud properties.

Through careful data analysis and comparison with theoretical models, we seek to understand the diversity of planetary climates and the formation history of substellar objects.