Panchromatic spectral energy distributions ofHerschelsources

S. Berta(Institut de Radioastronomie Millimétrique), L. Wang(University of Sussex), D. J. Rosario(Max Planck Society), D. Scott(University of British Columbia), F. Pozzi(University of Bologna), M. Viero(Kavli Institute for Particle Astrophysics and Cosmology), Seb Oliver(University of Sussex), D. Lutz(Max Planck Institute for Extraterrestrial Physics), E. Le Floc’h(Centrum Badań Kosmicznych), Ho Seong Hwang(Centre National de la Recherche Scientifique), A. Franceschini(University of Padua), Stijn Wuyts(University of Bath), E. Hatziminaoglou(European Southern Observatory), Asantha Cooray(University of California, Irvine), C. Gruppioni(Osservatorio di Astrofisica e Scienza dello Spazio), B. Magnelli(University of Bonn), I. Valtchanov(Commissariat à l'Énergie Atomique et aux Énergies Alternatives), P. Santini(Astronomical Observatory of Rome), L. Pozzetti(University of Bristol), L. Riguccini(Centre National de la Recherche Scientifique), D. Brisbin(Cornell University), R. Nordon(Max Planck Society), P. Popesso(Max Planck Society), M. Symeonidis(University College London), G. Rodighiero(University of Padua), I. G. Roseboom(University of Sussex), M. J. Page(University College London)

Astronomy and Astrophysics

January 18, 2013

Cited by 187

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Panchromatic spectral energy distributions of<i>Herschel</i>sources