THE COMPLEX PHYSICS OF DUSTY STAR-FORMING GALAXIES AT HIGH REDSHIFTS AS REVEALED BY<i>HERSCHEL</i>AND<i>SPITZER</i>
B. Lo Faro(Centre National de la Recherche Scientifique), Stijn Wuyts(University of Bath), M. J. Page(University College London), M. Vaccari(University of Cape Town), D. Scott(University of British Columbia), V. Buat(Centre National de la Recherche Scientifique), A. Feltre(Arcetri Astrophysical Observatory), D. Burgarella(Centre National de la Recherche Scientifique), Peter D. Hurley(University of Sussex), A. Cava(Universidad Complutense de Madrid), F. Pozzi(University of Bologna), L. Wang(University of Sussex), Seb Oliver(University of Sussex), D. Lutz(Max Planck Institute for Extraterrestrial Physics), D. Farrah(University of Sussex), A. Franceschini(University of Padua), G. Magdis(University of Copenhagen), D. L. Clements(Imperial College London), D. Rigopoulou(European University Cyprus), Asantha Cooray(University of California, Irvine), S. Berta(Institut de Radioastronomie Millimétrique), B. Magnelli(University of Bonn), M. Rowan-Robinson(Imperial College London), L. Silva(Trieste Astronomical Observatory), P. Popesso(Max Planck Society), A. J. Smith(University of Sussex), M. Symeonidis(University College London), J. J. Bock(Jet Propulsion Laboratory), I. G. Roseboom(University of Sussex), L. Marchetti(University of Padua), E. A. González Solares(University of Cambridge), G. Rodighiero(University of Padua)
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