tokens: We thank Mark Lacy for his advice and useful discussion with regards to the Sajina model, as well as George Helou for suggesting the extended Schmidt law as another point of analysis, and Yong Shi, Michael Brown, and Aditya Togi, whose comments improved the revised version of this paper. This work made use of the remote access computing accounts of the NASA Herschel Science Center, which were very helpful in reducing the Herschel data. L.L. and P.M.O. acknowledges support for this work provided by NASA through an award issued by JPL/Caltech. Support for K.A. is provided by NASA through Hubble Fellowship grant # HST -HF2-51352.001 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. This work is based in part on observations made with Herschel , a European Space Agency Cornerstone Mission with significant participation by NASA. This publication used observations made with the Spitzer Space Telescope , which is operated by the Jet Propulsion Laboratory (JPL)/California Institute of Technology (Caltech) under a contract with NASA. Observations from the Wide-field Infrared Survey Explorer , which is a joint project of the University of California, Los Angeles, and JPL/Caltech, funded by NASA, were also used. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center (IPAC)/Caltech, funded by NASA and the NSF, as well as from the Sloan Digital Sky Survey (Sloan-III), whose funding has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the NSF, and the U.S. DOE Office of Science, and which is managed by the Astrophysical Research Consortium for the Participating Institutions of the Sloan-III Collaboration. Finally, this publication makes use of data from the Galaxy Evolution Explorer , retrieved from the Mikulski Archive for Space Telescopes (MAST), part of the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non- HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. This research has made use of the NASA/IPAC Extragalactic Database (NED) and the Infrared Science Archive (IRSA) which are operated by the JPL/Caltech, under contract with the NASA, and NASA’s Astrophysics Data System (ADS). We also used software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. Facilities: Herschel , Spitzer , WISE , 2MASS , Sloan , GALEX .
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