<i>Herschel</i>PEP/HerMES: the redshift evolution (0 ≤<i>z</i>≤ 4) of dust attenuation and of the total (UV+IR) star formation rate density
D. Burgarella(Centre National de la Recherche Scientifique), M. Viero(Kavli Institute for Particle Astrophysics and Cosmology), F. Pozzi(University of Bologna), O. Cucciati(Osservatorio astronomico di Bologna), J. S. Dunlop(Royal Observatory), Seb Oliver(University of Sussex), D. Lutz(Max Planck Institute for Extraterrestrial Physics), E. Le Floc’h(Centrum Badań Kosmicznych), M. Béthermin(Centre National de la Recherche Scientifique), D. Farrah(University of Sussex), Asantha Cooray(University of California, Irvine), S. Heinis(Centre National de la Recherche Scientifique), S. Berta(Institut de Radioastronomie Millimétrique), C. Gruppioni(Osservatorio di Astrofisica e Scienza dello Spazio), B. Magnelli(University of Bonn), L. Riguccini(Centre National de la Recherche Scientifique), A. Franceschini(Osservatorio Astronomico di Padova), R. Nordon(Max Planck Society), P. Popesso(Max Planck Society), J. Böck(California Institute of Technology), M. Vaccari(University of Cape Town), M. J. Page(University College London), V. Buat(Centre National de la Recherche Scientifique)
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