Multi-wavelength lens reconstruction of a Planck and Herschel-detected star-bursting galaxy
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AST-1614213, NSF, National Science Foundation
We wish to thank the anonymous referee whose comments helped improve the paper. Financial support for this work was provided by NASA through grant HST-GO-13399 from the Space Telescope Science Institute, which is operated by Associated Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. Additional support for N.T., A. C., and H.N. was from NSF through AST-1313319. Some of the data presented herein 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. 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. The Submillimeter Array is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics and is funded by the Smithsonian Institution and the Academia Sinica. C.F. acknowledges funding from CAPES (proc. 12203–1). J.G.N. acknowledges financial support from the Spanish MINECO for a Ramon y Cajal fellowship. H.M.acknowledges support from the Fundação para a Ciência e a Tecnologia (FCT) through the Fellowship SFRH/BPD/ 97986/2013. I.O. acknowledges support from the European Research Council in the form of the Advanced Investigator Programme, 321302, COSMICISM. D.A.R. acknowledges support from the National Science Foundation under grant number AST-1614213 to Cornell University.
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