On the redshift evolution (0 < z < 4) of dust attenuation and of the total (UV+IR) star formation rate density
Le 17 mai 2013 À 10h30 Salle de Cours - Grande Coupole Denis BURGARELLA OAMP Marseille Using new homogeneous Luminosity Functions (LFs) in the FUV (VVDS) and in the FIR Herschel/PEP and Herschel/HerMES), we study the evolution of the dust attenuation with redshift. With this...