Groundbased and spacecraft telescopic observations, combined with an intensive modeling
effort, have greatly enhanced our understanding of hot giant planets and brown dwarfs over …

The ExoMol database (www. exomol. com) provides molecular data for spectroscopic
studies of hot atmospheres. These data are widely used to model atmospheres of …

Spectral retrieval has long been a powerful tool for interpreting planetary remote sensing
observations. Flexible, parameterised, agnostic models are coupled with inversion …

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 …

We present one of the most precise emission spectra of an exoplanet observed so far. We
combine five secondary eclipses of the hot Jupiter WASP-18b (T day∼ 2900 K) that we …

Hot Jupiters have been predicted to have a strong day/night temperature contrast and a
hotspot shifted eastward of the substellar point. This was confirmed by numerous phase …

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

In giant planet atmosphere modeling, the intrinsic temperature T int and radiative–
convective boundary (RCB) are important lower boundary conditions. Often in one …

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 future is now–after its long-awaited launch in 2021 December, JWST began science
operations in 2022 July and is already revolutionizing exoplanet astronomy. The Early …