Modeling the Radio to X-ray SED of Galaxies
  Our multi-wavelength model GRASIL for the SED of galaxies is described, in particular the recent extension to the radio and X-ray range. With our model we can study different aspects of galaxy evolution by exploiting all available spectral observations, where different emission components dominate. 
L. Silva, G.L. Granato, A. Bressan, P. Panuzzo