The 80 Ms follow-up of the X-ray afterglow of GRB 130427A challenges the standard forward shock model
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D. A. Kann | N. Gehrels | D. Malesani | G. Stratta | M. Boer | B. Gendre | Z. Cano | S. Schulze | E. Troja | M. Pasquale | S. Oates | L. Piro | B. Zhang | M. Page | A. Rossi | M. D. Pasquale | B. Zhang | B. Zhang | B. Zhang | B. Zhang | A. Rossi | Bing Zhang | S. Oates | S. Schulze | A. Rossi | M. Boër
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