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

Stellar, substellar, and planetary atmosphere models are all highly sensitive to the input
opacities. Generational differences between various state-of-the-art stellar/planetary models …

For decades, the remote sensing measurements have been made in planetary atmospheres
in the Solar System and beyond. As the performance of the space instruments improves, the …

This book presents a comprehensive overview of the modern theory of spectral line
broadening and shifting by pressure of atmospheric gases. It describes current semi …

An expression was developed that correctly models the temperature dependence of the half-
width over large temperature ranges and the temperature dependence of the line shift, even …

Opacities and chemical abundance data are crucial ingredients of ultracool dwarf and
extrasolar giant planet atmosphere models. We report here on the detailed sources of …

Temperature dependences of molecular line-shape parameters are important for the
spectroscopic studies of the atmospheres of the Earth and other planets. A number of …

Many atmospheres (cool stars, brown dwarfs, giant planets, extrasolar planets) are
predominately composed of molecular hydrogen and helium. H 2 16 O is one of the best …

Abstract The 20013–00001 and 20012–00001 bands of 12 C 16 O 2 in the 2 µm region are
used by many instruments on-board satellites and in ground-based networks to monitor the …

The goal of this white paper is to provide a snapshot of the data availability and data needs
primarily for the Ariel space mission, but also for related atmospheric studies of exoplanets …