UV properties and evolution of high-redshift galaxies
  I assess the problem of morphological and photometric evolution of high-redshift galaxies in the ultraviolet wavelength range. My discussion will partly rely on a new set of template galaxy models, in order to infer the expected changes along the Hubble morphological sequence at the different cosmic epochs. The impact of evolution on the faint-end galaxy luminosity function at z~1 and beyond will also be evaluated and briefly discussed. See http://www.merate.mi.astro.it/~eps/home.html for more info and model retrieval. 
Alberto Buzzoni (Telescopio Nazionale Galileo, La Palma, Spain, and   Oss. Astronomico di Brera, Milan Italy)