Update of the HITRAN collision-induced absorption section

Correct parameterization of the Collision-induced Absorption (CIA) phenomena is essential for accurate modeling of planetary atmospheres. The HITRAN spectroscopic database provides these parameters in a dedicated section. Here, we significantly revise and extend the HITRAN CIA data with respect to the original effort described in Richard et al. [JQSRT 113, 1276 (2012)]. The extension concerns new collisional pairs as well as wider spectral and temperature ranges for the existing pairs. The database now contains CIA for N-2-N-2, N-2-H-2, N-2-CH4, N-2-H2O, N-2-O-2, O-2-O-2, O-2-CO2, CO2-CO2, H-2-H-2, H-2-He, H-2-CH4, H-2-H, H-He, CH4-CH4, CH4-CO2, CH4-He, and CH4-Ar collision pairs. The sources of data as well as their validation and selection are discussed. A wish list to eliminate remaining deficiencies or lack of data from the astrophysics perspective is also presented.