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tokens: The authors thank the anonymous referee for useful comments and suggestions, which have improved this manuscript. Z.C.M. gratefully acknowledges support from the John F. Burlingame and the Kathryn McCarthy Graduate Fellowships in Physics at Tufts University. D.M. and Z.C.M. acknowledge the support of the Research Corporation for Science Advancement’s Cottrell Scholarship, the support from Tufts University Mellon Research Fellowship in Arts and Sciences. We thank Gabriela Calistro Rivera for her support on the implementation of AGNfitter . This study is partially based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under program ID 087.A-0514. Some of the data presented in this study were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. Keck telescope time was granted by NOAO, through the Telescope System Instrumentation Program (TSIP). TSIP is funded by NSF. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. This study makes use of data from the NEWFIRM Medium-Band Survey, a multi-wavelength survey conducted with the NEWFIRM instrument at the KPNO, supported in part by the NSF and NASA. We thank the NMBS and COSMOS collaborations for making their catalogs publicly available. The combination of NEWFIRM Medium-Band Survey and Herschel data was supported by the National Aeronautics and Space Administration (NASA) under grant number NNX13AH38G issued through the NNH12ZDA001N Astrophysics Data Analysis Program (ADAP).