The field of exoplanet atmospheric characterization has recently made considerable
advances with the advent of high-resolution spectroscopy from large ground-based …

Ultra-hot Jupiters are tidally locked gas giants with dayside temperatures high enough to
dissociate hydrogen and other molecules. Their atmospheres are vastly non-uniform in …

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

The near-infrared transmission spectrum of the warm sub-Neptune exoplanet GJ 1214 b has
been observed to be flat and featureless, implying a high metallicity atmosphere with …

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

The newly operational JWST offers the potential to study the atmospheres of distant worlds
with precision that has not been achieved before. One of the first exoplanets observed by …

The complexity of atmospheric retrieval models is largely data-driven, and one-dimensional
models have generally been considered adequate with current data quality. However …

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 …

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 …

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 …