PICASO-Lite Reference Data for the Roman Coronagraph School Europe

This particular combination of PICASO refrence data is meant to go along with the tutorial materials available here: https://github.com/blacy/picaso_for_roman_coronagraph_school They were prepared for the Roman Coronagraph School Europe in March 2026. They are meant to model giant planets and brown dwarfs ranging from internal temperatures of ~100 K up to 2400 K from wavelengths 0.4-7.0 microns at a low spectral resolution (~R=50), . Note that we include a library of direct imaging spectra and photometry compiled by Matthieu Ravet for a soon-to-be published paper, please credit him if you make use of them. They are referred to within the tutorials as the "EWI Database". We also make use of models from Batalha et al 2018 https://ui.adsabs.harvard.edu/abs/2018AJ....156..158B/abstract . The full PICASO documentation website is here: https://natashabatalha.github.io/picaso/ , which includes detailed instructions on installation.