Herschel reveals the obscured star formation in HiZELS H emitters at z = 1.47
E. Ibar(University of Valparaíso), M. Zemcov(Rochester Institute of Technology), N. Seymour, Ian Smail(Durham University), J. L. Wardlow, D. Lutz(Max Planck Institute for Extraterrestrial Physics), E. Le Floc’h(Centrum Badań Kosmicznych), P. N. Best(Royal Observatory), M. Béthermin(Centre National de la Recherche Scientifique), D. Farrah(University of Sussex), G. Magdis(University of Copenhagen), R. J. Ivison(Royal Observatory), Soh Ikarashi(The University of Tokyo), G. Marsden(University of British Columbia), V. Arumugam(Royal Observatory), S. Berta(Institut de Radioastronomie Millimétrique), B. Magnelli(University of Bonn), David Sobral(Lancaster University), Kotaro Kohno(The University of Tokyo), J. J. Bock(California Institute of Technology), M. Symeonidis(University College London), S. J. Oliver(University of Sussex), A. J. Smith(University of Sussex), M. J. Page(University College London), L. Riguccini(Centre National de la Recherche Scientifique), F. Pozzi(Osservatorio astronomico di Bologna), A. Conley(Laboratory for Atmospheric and Space Physics), B. Schulz(California Institute of Technology), J. E. Geach(University of Hertfordshire), L. Wang(University of Sussex), A. Cava(Universidad Complutense de Madrid)
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