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HITRAN in the XXIst century: beyond Voigt and beyond EarthHITRAN in the XXIst century: beyond Voigt and beyond Earth

HITRAN application programming interface (HAPI): A comprehensive approach to working with spectroscopic dataThe HITRAN Application Programming Interface (HAPI) is presented. HAPI is a free Python library

Working with HITRAN database using HAPI: HITRAN Application Programming InterfaceWorking with HITRAN database using HAPI: HITRAN Application Programming Interface

Working with the HITRAN database using HAPI: HITRAN Application Programming InterfaceWorking with the HITRAN database using HAPI: HITRAN Application Programming Interface

Introduction to HITRAN Application Programming Interface (HAPI)Introduction to HITRAN Application Programming Interface (HAPI)

Non-Voigt line-shape analysis of H2 spectra for the HITRAN databaseNon-Voigt line-shape analysis of H2 spectra for the HITRAN database

Addition to the HITRAN database of line-shape parameters due to the pressure of H2, He and CO2. Part 1: SO2, NH3, HF, HCL, OCS and C2H2Addition to the HITRAN database of line-shape parameters due to the pressure of H2, He and CO2

HITRANonline: A new structure and interface for HITRAN line lists and cross sectionsHITRANonline: A new structure and interface for HITRAN line lists and cross sections

Infrared spectra of 16O3 in the 900-5600 cm-1 range revisited: Empirical corrections to the S&MPO and HITRAN2020 line lists&MPO and HITRAN2020 line lists

H2, He, and CO2 line-broadening coefficients, pressure shifts and temperature-dependence exponents for the HITRAN database. Part 1: SO2, NH3, HF, HCl, OCS and C2H2To increase the potential for use of the HITRAN database in astronomy, experimental and theoretical

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