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

This review covers the work of the three decades since the first spectroscopic identification
of the H 3+ molecular ion outside of the laboratory in 1988, in the auroral atmosphere of the …

The ExoMol database (www. exomol. com) provides extensive line lists of molecular
transitions which are valid over extended temperature ranges. The status of the current …

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 …

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 majority of stars are now thought to support exoplanets. Many of those exoplanets
discovered thus far are categorized as rocky objects with an atmosphere. Most of these …

EXOCROSS is a Fortran code for generating spectra (emission, absorption) and
thermodynamic properties (partition function, specific heat, etc.) from molecular line lists …

Transmission spectroscopy is one of the premier methods used to probe the temperature,
composition, and cloud properties of exoplanet atmospheres. Recent studies have …

Updated Low-temperature Gas Opacities with ÆSOPUS 2.0 - IOPscience This site uses
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …