picaso enables the: 1) computation of exoplanet and brown dwarf spectroscopy in transmission, emission or reflected light, 2) 1D climate modeling of brown dwarfs and exoplanets, 3) fitting spectroscopic data to models.
Reflected Light Spectroscopy of planets
Thermal Emission Spectroscopy of planets and brown dwarfs
Transit Spectroscopy of planets
Phase Curves of planets
1D Climate modeling of planets and brown dwarfs
Fitting models to data