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

This review presents an insight into our current knowledge of the atmospheres of the planets
Venus, Mars, Jupiter, Saturn, Uranus and Neptune, the satellite Titan, and those of …

The abundance of refractory elements in giant planets can provide key insights into their
formation histories. Owing to the low temperatures of the Solar System giants, refractory …

Ground-based high-resolution spectroscopy (HRS) has detected numerous chemical
species and atmospheric dynamics in exoplanets, most notably ultrahot Jupiters (UHJs) …

The computation of complex neutral/ionized chemical equilibrium compositions is invaluable
to obtain scientific insights of, for example, the atmospheres of extrasolar planets and cool …

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

Ultra-hot Jupiters are tidally locked with their host stars, dividing their atmospheres into a hot
dayside and a colder nightside. As the planet moves through transit, different regions of the …

We present high-resolution dayside thermal emission observations of the exoplanet WASP-
18 b using IGRINS on Gemini South. We remove stellar and telluric signatures using …

Relating planet formation to atmospheric composition has been a long-standing goal of the
planetary science community. So far, most modeling studies have focused on predicting the …

The new hyperfine-resolved HyVO line lists for vanadium monoxide (51V16O) are
presented. The new line list considers 15 electronic states and comprises almost 59 billion …