HITRAN Application Programming Interface (HAPI): A comprehensive approach to working with spectroscopic data

By R. Kochanov, I. Gordon, L. Rothman, P. Wcisło, Christian Hill, J. Wilzewski. 2016

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An Accurate, Extensive, and Practical Line List of Methane for the HITEMP Database (2020, methodology): “The resulting HITEMP line list from this work can be compared to high-resolution absorption cross-sections of HITRAN2016 at 296 K, calculated using the HAPI routines (Kochanov et al. 2016).”
Update of the HITRAN collision-induced absorption section (2019, unknown): “Access through the HITRAN Application Programming Interface (HAPI) (Kochanov et al., 2016) will also be enabled.”
The GHGSat-D imaging spectrometer (2020, methodology): “Tech., 14, 2127–2140, 2021 the light travels through the atmosphere with respect to the Earth’s surface normal; z is the altitude; αabs is the pressure-, temperature-, wavelength-, and species-dependent absorption coefficient calculated using the HITRAN API (Kochanov et al., 2016); and the solar irr”