A HIGHER EFFICIENCY OF CONVERTING GAS TO STARS PUSHES GALAXIES AT <i>z</i> ∼ 1.6 WELL ABOVE THE STAR-FORMING MAIN SEQUENCE
J. D. Silverman(Kavli Institute for the Physics and Mathematics of the Universe), G. Zamorani(Osservatorio di Astrofisica e Scienza dello Spazio), A. Renzini(Osservatorio Astronomico di Padova), Tohru Nagao(Ehime University), C. Feruglio(Institut de Radioastronomie Millimétrique), C. Mancini(University of Padua), Anton M. Koekemoer(Space Telescope Science Institute), D. Lutz(Max Planck Institute for Extraterrestrial Physics), M. Béthermin(Centre National de la Recherche Scientifique), N. Arimoto(The Graduate University for Advanced Studies, SOKENDAI), G. Magdis(University of Copenhagen), W. Rujopakarn(Chulalongkorn University), E. Daddi(Centre National de la Recherche Scientifique), S. Berta(Institut de Radioastronomie Millimétrique), Daichi Kashino(Nagoya University), M. Sargent(University of Sussex), Jeyhan S. Kartaltepe(Kitt Peak National Observatory), Masato Onodera(ETH Zurich), Daizhong Liu(Unknown), D. B. Sanders(University of Hawaii System)
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