Calculations are reported on the rotation-vibration energy levels of the arsine molecule with associated transition intensities. A potential energy surface (PES) obtained from ab initio electronic structure calculations is refined to experimental data, and the resulting energy levels display subwavenumber accuracy for all reliably known J = 0 term values under 6500 cm −1 . After a small empirical adjustment of the band centres, our calculated (J = 1 − 6) rovibrational states reproduce 578 experimentally derived energies with a root-mean-square error of 0.122 cm −1 . Absolute line intensities are computed using the refined PES and a new dipole moment surface (DMS) for transitions between states with energies up to 10 500 cm −1 and rotational quantum number J = 30.The computed DMS reproduces experimental line intensities to within 10% uncertainty for the ν 1 and ν 3 bands. Furthermore, our calculated absorption cross-sections display good agreement with the main absorption features recorded in Pacific Northwest National Laboratory (PNNL) for the complete range of 600 − 6500 cm −1 .Considering the unsuitability of the current state of AsH 3 data for either exoplanet modelling, which necessitates completeness, or industrial monitoring, which necessitates accuracy, we decided to construct a comprehensive line list for arsine which could be used for the applications mentioned above. Our approach to constructing linelists, as exploited in the ExoMol project 26,27 , uses potential energy surfaces which have been refined using spectroscopic data but ab initio dipole moment surfaces, which have J o u r n a l N a me , [ y e a r ] , [ v o l . ] , 1-15 | 1