Deep observations of CO line emission from star-forming galaxies in a cluster candidate atz=1.5

Manuel Aravena, F. Pozzi(Osservatorio astronomico di Bologna), F. Bertoldi, A. Finoguenov(Max Planck Institute for Extraterrestrial Physics), Dominik A. Riechers(Cornell University), L. Lentati, M. Salvato(Max Planck Society), Seb Oliver(University of Sussex), Eva Schinnerer(Max Planck Institute for Astronomy), C. L. Carilli(National Radio Astronomy Observatory), D. Lutz(Max Planck Institute for Extraterrestrial Physics), S. C. Chapman(University of Warwick), L. Riguccini(Ames Research Center), D. Farrah(University of Sussex), G. Magdis(University of Copenhagen), S. Berta(Institut de Radioastronomie Millimétrique), B. Magnelli(University of Bonn), P. Capak(California Institute of Technology), Masaomi Tanaka(National Astronomical Observatory of Japan), V. Smolčić(University of Zagreb), E. Le Floc’h(Centrum Badań Kosmicznych), Fabian Walter(California Institute of Technology)

Monthly Notices of the Royal Astronomical Society

September 12, 2012

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Deep observations of CO line emission from star-forming galaxies in a cluster candidate at<i>z</i>=1.5