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The ExoMol project: Software for computing large molecular line lists

The use of variational nuclear motion programs to compute line lists of transition frequencies and intensities is now a standard procedure. The ExoMol project has used this technique to generate line lists for studies of hot bodies such as the atmospheres of exoplanets and cool stars. The resulting line list can be huge: many contain 10 billion or more transitions. This software update considers changes made to our programs during the course of the project to allow for such calculations. This update considers three programs: {\sc Duo} which computed vibronic spectra for diatomics, {\sc DVR3D} which computes rotation-vibration spectra for triatomics, and {\sc TROVE} which computes rotation-vibration spectra for general polyatomic systems. Important updates in functionality include the calculation of quasibound (resonance) states and Landé $g$-factors by {\sc Duo} and the calculation of resonance states by {\sc DVR3D}. Significant algorithmic improvements are reported for both {\sc DVR3D} and {\sc TROVE}. All three programs are publically available from ccpforge.cse.rl.ac.uk. Future developments are also considered.