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SN2017jgh: A high-cadence complete shock cooling light curve of a SN IIb with the Kepler telescope

  • P. Armstrong*
  • , B. E. Tucker*
  • , A. Rest*
  • , R. Ridden-Harper
  • , Y. Zenati
  • , A. L. Piro
  • , S. Hinton
  • , C. Lidman
  • , S. Margheim
  • , G. Narayan
  • , E. Shaya
  • , P. Garnavich
  • , D. Kasen
  • , V. Villar
  • , A. Zenteno
  • , I. Arcavi
  • , M. Drout
  • , R. J. Foley
  • , J. Wheeler
  • , J. Anais
    • A. Campillay, D. Coulter, G. Dimitriadis, D. Jones, C. D. Kilpatrick, N. Muñoz-Elgueta, C. Rojas-Bravo, J. Vargas-González, J. Bulger, K. Chambers, M. Huber, T. Lowe, E. Magnier, B. J. Shappee, S. Smartt, K. W. Smith, T. Barclay, G. Barentsen, J. Dotson, M. Gully-Santiago, C. Hedges, S. Howell, A. Cody, K. Auchettl, A. Bódi, Zs Bognár, J. Brimacombe, P. Brown, B. Cseh, L. Galbany, D. Hiramatsu, T. W.S. Holoien, D. A. Howell, S. W. Jha, R. Könyves-Tóth, L. Kriskovics, C. McCully, P. Milne, J. Muñoz, Y. Pan, A. Pál, H. Sai, K. Sárneczky, N. Smith, Sódor, R. Szabó, R. Szakáts, S. Valenti, J. Vinkó, X. Wang, K. Zhang, G. Zsidi
*Corresponding author for this work

    Research output: Contribution to journal › Article › peer-review

    18 Citations (Scopus)

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