VALIDATION OF THE EQUILIBRIUM MODEL FOR GALAXY EVOLUTION TO<i>z</i>∼ 3 THROUGH MOLECULAR GAS AND DUST OBSERVATIONS OF LENSED STAR-FORMING GALAXIES
A. Saintonge(Max Planck Institute for Extraterrestrial Physics), Stijn Wuyts(University of Bath), R. Genzel(Max Planck Institute for Extraterrestrial Physics), A. J. Baker(Rutgers, The State University of New Jersey), D. Lutz(Max Planck Institute for Extraterrestrial Physics), E. Sturm(Max Planck Institute for Extraterrestrial Physics), K. Bandara(Max Planck Institute for Extraterrestrial Physics), S. Berta(Institut de Radioastronomie Millimétrique), B. Magnelli(University of Bonn), L. J. Tacconi(Max Planck Institute for Extraterrestrial Physics), N. M. Förster Schreiber(Max Planck Institute for Extraterrestrial Physics), Eva Wuyts(Max Planck Institute for Extraterrestrial Physics), Raanan Nordon(Max Planck Institute for Extraterrestrial Physics), A. Poglitsch(Max Planck Institute for Extraterrestrial Physics)
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