GALAXY STRUCTURE AND MODE OF STAR FORMATION IN THE SFR-MASS PLANE FROMz∼ 2.5 TOz∼ 0.1

Stijn Wuyts(University of Bath), L. J. Tacconi(Max Planck Institute for Extraterrestrial Physics), A. Cava(Universidad Complutense de Madrid), F. Pozzi(University of Bologna), Elizabeth J. McGrath(Colby College), Nimish P. Hathi(Space Telescope Science Institute), R. Genzel(Max Planck Institute for Extraterrestrial Physics), A. Saintonge(Max Planck Institute for Extraterrestrial Physics), Anton M. Koekemoer(Space Telescope Science Institute), D. Lutz(Max Planck Institute for Extraterrestrial Physics), E. Le Floc’h(Centrum Badań Kosmicznych), Guillermo Barro(University of the Pacific), Yicheng Guo(Army Medical University), Kyoung-Soo Lee(Purdue University West Lafayette), S. Berta(Institut de Radioastronomie Millimétrique), Dale D. Kocevski(Colby College), B. Magnelli(University of Bonn), Arjen van der Wel(Federal Foreign Office), Kuang-Han Huang(Johns Hopkins University), N. M. Förster Schreiber(Max Planck Institute for Extraterrestrial Physics), Raanan Nordon(Max Planck Institute for Extraterrestrial Physics), Laurie A. Riguccini(Centre National de la Recherche Scientifique), G. Rodighiero(University of Padua), Paola Popesso(Max Planck Institute for Extraterrestrial Physics), J. Graciá‐Carpio(Max Planck Institute for Extraterrestrial Physics)

The Astrophysical Journal

November 11, 2011

Cited by 744

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GALAXY STRUCTURE AND MODE OF STAR FORMATION IN THE SFR-MASS PLANE FROM<i>z</i>∼ 2.5 TO<i>z</i>∼ 0.1