Gaia17biu/SN 2017egm in NGC 3191: The Closest Hydrogen-poor Superluminous Supernova to Date Is in a "Normal," Massive, Metal-rich Spiral Galaxy

Research output: Contribution to journalJournal articleResearchpeer-review

  • 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 Lundqvist
  • Seppo 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
  • 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
Original languageEnglish
Article number57
JournalAstrophysical Journal
Volume853
Issue number1
Number of pages20
ISSN0004-637X
DOIs
Publication statusPublished - 20 Jan 2018

    Research areas

  • galaxies: individual (NGC 3191), supernovae: general, supernovae: individual (SN 2017egm Gaia17biu)

Links

ID: 200677533