Padova-Asiago Supernova Group
Giorgio Valerin

My main research interests include different classes of hydrogen rich transients, which share the peculiarity of being underluminous compared to standard type II supernovae (SNe II). I am particularly keen on the modeling and physical interpretation of light curves and spectra obtained in the ultraviolet, optical and infrared domains. The starting point of my studies was a category of faint SNe: