The HITRAN database is a compilation of molecular spectroscopic parameters. It was
established in the early 1970s and is used by various computer codes to predict and …

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

ABSTRACT A new line list for HO is presented. This line list, which is called POKAZATEL,
includes transitions between rotational–vibrational energy levels up to 41 000 cm− 1 and is …

Accurate line lists are crucial for correctly modelling a variety of astrophysical phenomena,
including stellar photospheres and the atmospheres of extrasolar planets. This paper …

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 …

The GEISA database (Gestion et Etude des Informations Spectroscopiques Atmosphériques:
Management and Study of Atmospheric Spectroscopic Information) has been developed …

Total internal partition sums (TIPS) are reported for 166 isotopologues of 51 molecules
important in planetary atmospheres. Molecules 1 to 50 are taken from the HITRAN2016 list …

Y dwarfs are the coolest spectral class of brown dwarf. They have effective temperatures
less than 500 K, with the coolest detection as low as∼ 250 K. They make up the low-mass …

ABSTRACT A new ro-vibrational line list for the ground electronic state of the main
isotopologue of acetylene, 12C2H2, is computed as part of the ExoMol project. The aCeTY …