Paper: 2016ApJ...833..156U (acknowledgments)
We thank the anonymous referee for a careful reading of the manuscript and insightful suggestions. We are very grateful to all of the Subaru Telescope staff. We thank Dr. Furusawa for providing the Suprime-Cam number counts we used to check our data. We thank Dr. Hamana for providing his reconstruction code. We thank Dr. Oguri for incisive comments that have led to improvements in the analysis and discussion. We thank Dr. Okabe for sharing computer resources necessary for reduction and analysis. We thank Dr. Barnacka for a careful reading of the manuscript. Y.U. was supported by a Grant-in-Aid for Young Scientists (B) from the JSPS (26800103) and MEXT Grant-in-Aid for Scientific Research on Innovative Areas New Developments in Astrophysics Through Multi-Messenger Observations of Gravitational Wave Sources (24103003). The Smithsonian Institution supports the research of M.J.G. A Smithsonian Clay Postdoctoral Fellowship generously supports the research of H.J.Z. The Hyper Suprime-Cam (HSC) collaboration includes the astronomical communities of Japan and Taiwan, and Princeton University. The HSC instrumentation and software were developed by the National Astronomical Observatory of Japan (NAOJ), the Kavli Institute for the Physics and Mathematics of the universe (Kavli IPMU), the University of Tokyo, the High Energy Accelerator Research Organization (KEK), the Academia Sinica Institute for Astronomy and Astrophysics in Taiwan (ASIAA), and Princeton University. Funding was contributed by the Ministry of Education, Culture, Sports, Science and Technology (MEXT), the Japan Society for the Promotion of Science (JSPS), (Japan Science and Technology Agency (JST), the Toray Science Foundation, NAOJ, Kavli IPMU, KEK, ASIAA, and Princeton University. We used software developed for the Large Synoptic Survey Telescope. We thank the LSST Project for making their code available as free software at http://dm.lsstcorp.org (Ivezic et al. 2008 ; Axelrod et al. 2010 ). We acknowledge the use of lensfit for shear measurement (Miller et al. 2007 ; Kitching et al. 2008 ). Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/ . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this sacred mountain. Facilities: Subaru (HSC) , MMT (Hectospec).