THE AFTERGLOW OF GRB 130427A FROM 1 TO 10<sup>16</sup>GHz

A. Perley, D.; B. Cenko, S.; Corsi, A.; R. Tanvir, N.; J. Levan, A.; А. Канн, Д.; Сонбас, Э.; Wiersema, K.; Zheng, WeiKang; Zhao, Xiaohong; M. Bai, J.; Bremer, Michael; J. Castro‐Tirado, A.; Chang, Liang; I. Clubb, K.; A. Frail, D.; S. Fruchter, A.; Göğüş, Ersin; Greiner, J.; Güver, Tolga; Horesh, A.; V. Filippenko, A.; Klose, S.; Mao, J.; N. Morgan, A.; Pozanenko, A.; Schmidl, S.; Stecklum, B.; Tanga, M.; Volnova, A.; E. Volvach, A.; Wang, J.-G.; M. Winters, J.; Xin, Yu

doi:10.1088/0004-637x/781/1/37

Public

THE AFTERGLOW OF GRB 130427A FROM 1 TO 10<sup>16</sup>GHz

Shared by NobleBlocks on Jan 6, 2014 • 12:00 AM UTC

Authors:

D. A. Perley

S. B. Cenko

A. Corsi

Abstract

We present multiwavelength observations of the afterglow of GRB 130427A, the brightest (in total fluence) gamma-ray burst (GRB) of the past 29 yr. Optical spectroscopy from Gemini-North reveals the redshift of the GRB to be z = 0.340, indicating that its unprecedented brightness is primarily the res...

Subject

Afterglow

Gamma-ray burst

Astrophysics

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