Measuring the abundances of carbon and oxygen in exoplanet atmospheres is considered a
crucial avenue for unlocking the formation and evolution of exoplanetary systems,. Access to …

Measuring the metallicity and carbon-to-oxygen (C/O) ratio in exoplanet atmospheres is a
fundamental step towards constraining the dominant chemical processes at work and, if in …

Population studies of exoplanets are key to unlocking their statistical properties. So far, the
inferred properties have been mostly limited to planetary, orbital, and stellar parameters …

We present analysis of the atmospheres of 70 gaseous extrasolar planets via transit
spectroscopy with Hubble's Wide Field Camera 3 (WFC3). For over half of these, we …

Giant planets can interact with multiple and chemically diverse environments in
protoplanetary disks while they form and migrate to their final orbits. The way this interaction …

We have entered the era of the James Webb Space Telescope (JWST). We use the first
JWST transmission spectrum of the hot Saturn-mass exoplanet, WASP-39 b, obtained with …

Aims. Our goal is to create a retrieval framework which encapsulates the three-dimensional
(3D) nature of exoplanet atmospheres, and to apply it to observed emission phase curve …

Brown dwarfs serve as ideal laboratories for studying the atmospheres of giant exoplanets
on wide orbits, as the governing physical and chemical processes within them are nearly …

Photochemistry is expected to change the chemical composition of the upper atmospheres
of irradiated exoplanets through the dissociation of species, such as methane and ammonia …

The atmospheric C/O ratio of exoplanets is widely used to constrain their formation. To
guarantee that the C/O ratio provides robust information, we need to accurately quantify the …