Advances in the development of quantum chemical methods and progress in multicore
architectures in computer science made the simulation of infrared spectra of isolated …

Measuring the abundances of carbon and oxygen in exoplanet atmospheres is considered a
crucial avenue for unlocking the formation and evolution of exoplanetary systems,. Access to …

The abundances of main carbon-and oxygen-bearing gases in the atmospheres of giant
exoplanets provide insights into atmospheric chemistry and planet formation processes …

Measurements of the atmospheric carbon (C) and oxygen (O) relative to hydrogen (H) in hot
Jupiters (relative to their host stars) provide insight into their formation location and …

The recent inference of sulfur dioxide (SO2) in the atmosphere of the hot (approximately
1,100 K), Saturn-mass exoplanet WASP-39b from near-infrared JWST observations …

A set of empirical rovibrational energy levels, obtained through the MARVEL (measured
active rotational‐vibrational energy levels) procedure, is presented for the 13 C 16 O 2 …

Hot Jupiters are among the best-studied exoplanets, but it is still poorly understood how their
chemical composition and cloud properties vary with longitude. Theoretical models predict …

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

Here we present a publicly available database of opacities for molecules of astrophysical
interest named ExoMolOP that has been compiled for over 80 species, and is based on the …

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 …