THE IMPACT OF EVOLVING INFRARED SPECTRAL ENERGY DISTRIBUTIONS OF GALAXIES ON STAR FORMATION RATE ESTIMATES
R. Nordon(Max Planck Society), Lin Yan(California Institute of Technology), A. Poglitsch(Max Planck Institute for Extraterrestrial Physics), J. Cepa(Instituto de Astrofísica de Canarias), P. Andreani(European Southern Observatory), D. J. Rosario(Max Planck Society), R. Maiolino(University of Cambridge), F. Pozzi(University of Bologna), R. Genzel(Max Planck Institute for Extraterrestrial Physics), G. Lagache(Centre National de la Recherche Scientifique), D. Fadda(California Institute of Technology), A. Saintonge(Max Planck Institute for Extraterrestrial Physics), M. Sánchez‐Portal(European Space Astronomy Centre), D. Lutz(Max Planck Institute for Extraterrestrial Physics), E. Sturm(Max Planck Institute for Extraterrestrial Physics), B. Altieri(European Space Astronomy Centre), Stijn Wuyts(University of Bath), E. Daddi(Centre National de la Recherche Scientifique), S. Berta(Institut de Radioastronomie Millimétrique), B. Magnelli(University of Bonn), I. Valtchanov(Commissariat à l'Énergie Atomique et aux Énergies Alternatives), L. J. Tacconi(Max Planck Institute for Extraterrestrial Physics), P. Santini(Astronomical Observatory of Rome), A. Cimatti, N. M. Förster Schreiber(Max Planck Institute for Extraterrestrial Physics), A. M. Pérez García(Harvard University Press), Á. Bongiovanni, P. Popesso(Max Planck Society), G. Rodighiero(University of Padua)
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