Constraining planet formation based on the atmospheric composition of exoplanets is a
fundamental goal of the exoplanet community. Existing studies commonly try to constrain …

Hot giant exoplanets are very exotic objects with no equivalent in the Solar System that
allow us to study the behavior of atmospheres under extreme conditions. Their thermal and …

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 …

Ground-based high-resolution transmission spectroscopy has emerged as a promising
technique for detecting chemicals in transiting exoplanetary atmospheres. Despite chemical …

Context. High-resolution spectroscopy studies of ultra-hot Jupiters have been key in our
understanding of exoplanet atmospheres. Observing into the atmospheres of these giant …

The dayside atmospheres of ultra-hot Jupiters (UHJs) are predicted to possess temperature
inversion layers with extremely high temperatures at high altitudes. We observed the …

Ultra-hot Jupiters are perfect targets for transmission spectroscopy. However, their
atmospheres feature strong spatial variations in temperature, chemistry, dynamics, cloud …

Exoplanet atmosphere studies are often enriched by synergies with brown dwarf analogs.
However, many key molecules commonly seen in brown dwarfs have yet to be confirmed in …

Ultra-hot Jupiters are highly irradiated gas giant exoplanets on close-in orbits around their
host stars. The dayside atmospheres of these objects strongly emit thermal radiation due to …

Due to their likely tidally synchronized nature,(ultra) hot Jupiter atmospheres should
experience strongly spatially heterogeneous instellation. The large irradiation contrast and …