Gaia17biu/SN 2017egm in NGC 3191: The Closest Hydrogen-poor Superluminous Supernova to Date Is in a "Normal," Massive, Metal-rich Spiral Galaxy
Subhash Bose, Subo Dong, A. Pastorello, Alexei V. Filippenko, C. S. Kochanek, Jon Mauerhan, C. Romero-Canizales, Thomas G. Brink, Ping Chen, J. L. Prieto, R. Post, Christopher Ashall, Dirk Grupe, L. Tomasella, Stefano Benetti, B. J. Shappee, K. Z. Stanek, Zheng Cai, E. Falco, Peter LundqvistSeppo Mattila, Robert Mutel, Paolo Ochner, David Pooley, M. D. Stritzinger, S., Jr. Villanueva, WeiKang Zheng, R. J. Beswick, Peter J. Brown, E. Cappellaro, Scott Davis, Morgan Fraser, Thomas de Jaeger, N. Elias-Rosa, C. Gall, B. Scott Gaudi, Gregory J. Herczeg, Julia Hestenes, T. W. -S. Holoien, Griffin Hosseinzadeh, E. Y. Hsiao, Shaoming Hu, Shin Jaejin, Ben Jeffers, R. A. Koff, Sahana Kumar, Alexander Kurtenkov, Marie Wingyee Lau, Simon Prentice, T. Reynolds, Richard J. Rudy, Melissa Shahbandeh, Auni Somero, Keivan G. Stassun, Todd A. Thompson, Stefano Valenti, Jong-Hak Woo, Sameen Yunus
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