We provide a brief review of many aspects of the planetary physics of hot Jupiters. Our aim is
to cover most of the major areas of current study while providing the reader with additional …

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

The emergent spectra of close-in, giant exoplanets ('hot Jupiters') are expected to be distinct
from those of self-luminous objects with similar effective temperatures because hot Jupiters …

Abstract Upcoming James Webb Space Telescope observations will allow us to study
exoplanet and brown dwarf atmospheres in great detail. The physical interpretation of these …

Observations of exoplanet atmospheres have shown that aerosols, like in the solar system,
are common across a variety of temperatures and planet types. The formation and …

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

Context. Ultra-hot Jupiters are the hottest exoplanets that have been discovered so far.
Observations begin to provide insight into the composition of their extended atmospheres …

We report the first detection of CO emission at high spectral resolution in the day-side
infrared thermal spectrum of an exoplanet. These emission lines, found in the atmosphere of …

Radiative-transfer (RT) is a fundamental part of modelling exoplanet atmospheres with
general circulation models (GCMs). An accurate RT scheme is required for estimates of the …

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 …