Here is a list of the physical and chemical input data used by ProDiMo
- line lists, energies, statistical weights, and collisional data
- Leiden Lamda
- HITRAN 2020 and HITEMP
- CHIANTI database
- H2 ro-vibronic data
- CO ro-vibronic data (Chandra et al., …)
- Leiden Lamda
- chemical reaction rates
- UMIST 2012
- KIDA 2014
- OSU (deprecated, kept for benchmarking)
- STAND 2020 (reaction network for planetary chemistry, P. Rimmer)
- UMIST 2012
- desorption energies
- UMIST
- other sources (Garrod, Penteado)
- thermochemical data
- UMIST (heat of formation at 0K)
- BURCAT (temperature-dependent enthalpies and Gibb's free energies)
- UMIST (heat of formation at 0K)
- Photodissociation and photoionisation
- Stellar spectra:
- Kurucz
- Phoenix new generation
- Drift-Phoenix for brown dwarfs
- Photometric filters:
- various sources, about 650 filter transmission files
- various sources, about 650 filter transmission files
- dust and ice optical constants:
- various sources (papers, books, databases), about 150 materials
- various sources (papers, books, databases), about 150 materials
- PAH opacities
- Li & Draine (2001) with updates from Draine & Li (2007)
- Xray - gas cross-sections
- xraylib , Schoonjans et al. 2011 (absorption and scattering)
- Verner et al. (1995), Verner et al. (1996) (absorption)