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 …

The ExoMol project is dedicated to providing molecular line lists for exoplanet and other hot
atmospheres. The ExoMol procedure uses a mixture of ab initio calculations and available …

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 …

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 …

The water vapor line at 183 GHz was studied over the temperature range of 219–358 K
using a spectrometer with radioacoustic detection of absorption, providing a signal-to-noise …

A series of spectra of the quadrupolar electric S (2) transition of H2 in the 1–0 band near
4917 cm− 1 has been recorded at seven pressure values between 2 and 100 Torr. The …

A series of spectra, one pure H2O and four H2O-O2 mixtures, were measured for the ν2
band in the 1200–1950 cm− 1 region at room temperature using a single-pass copper cell …

In a recent work [JQSRT 228, 79 (2019)], Vispoel et al. optimized the intermolecular potential
used in the Modified Complex Robert-Bonamy (MCRB) formalism for the H 2 ON 2 collision …

Abstract Modified Complex Robert-Bonamy (MCRB) calculations of the half-width, line shift,
and their temperature dependence were made for the H 2 ON 2 collision system. Several …

Abstract Modified Complex Robert-Bonamy calculations were made for the CO 2-H 2 O
collision system using an intermolecular potential comprised of quadrupole-dipole …