Transport-induced quenching, ie the homogenization of chemical abundances by
atmospheric advection, is thought to occur in the atmospheres of hot gas giant exoplanets …

Stellar flares present challenges to the potential habitability of terrestrial planets orbiting M
dwarf stars through inducing changes in the atmospheric composition and irradiating the …

The atmospheres of ultra-hot Jupiters have been characterized in detail through recent
phase curve and low-and high-resolution emission and transmission spectroscopic …

Insight into the formation and global distribution of cloud particles in exoplanet atmospheres
continues to be a key problem to tackle going into the JWST era. Understanding …

Simulations with a 3D general circulation model (GCM) suggest that one potential driver
behind the observed radius inflation in hot Jupiters may be the downward advection of …

Context. Optical secondary eclipse measurements of small planets can provide a wealth of
information about the reflective properties of these worlds, but the measurements are …

Context. The chemical inventory of hot Jupiter (HJ) exoplanet atmospheres continues to be
observed by various ground-and space-based instruments in increasing detail and …

Context. Stellar flares of active M dwarfs can affect the atmospheric composition of close-
orbiting gas giants, and can result in time-dependent transmission spectra. Aims. We aim to …

The atmospheres of ultra hot Jupiters (UHJs) are prime targets for the detection of molecules
and atoms at both low and high spectral resolution. We study the atmospheres of the UHJs …

We present new functionality within PICASO, a state-of-the-art radiative transfer model for
exoplanet and brown dwarf atmospheres, by developing a new pipeline that computes …