Super-Eddington Accretion in the WISE-selected Extremely Luminous Infrared Galaxy W2246-0526

The authors gratefully acknowledge the anonymous referee for valuable comments and suggestions that improved the paper. C.-W.T. would like to thank Jian-Min Wang for the valuable discussions. This material is based upon work supported by the National Aeronautics and Space Administration under proposal 13-ADAP13-0092 issued through the Astrophysics Data Analysis Program. H.D.J. is supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education (NRF-2017R1A6A3A04005158). J.W. is supported by the National Key Program for Science and Technology Research and Development of China (grant 2016YFA0400702) and project 11673029 supported by NSFC. R.J.A. was supported by FONDECYT grant 1151408. T.D.-S. acknowledges support from ALMA-CONICYT project 31130005 and FONDECYT regular project 1151239. This publication makes use of data obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among Caltech, the University of California, and NASA. The Keck 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 Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory, California Institute of Technology, funded by the National Aeronautics and Space Administration. This research has made use of the NASA/IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. Facilities: Keck:I (OSIRIS - , LRIS) - , Herschel Space Te