Pak-Hin Thomas Tam, Qing-Wen Tang, Shujing Hou, Ruo-Yu Liu, Xiang-Yu Wang
The extended high-energy gamma-ray (>100 MeV) emission occurred after the prompt gamma-ray bursts is usually characterized by a single power-law spectrum, which has been explained as the afterglow synchrotron radiation. The afterglow inverse-Compton emission has long been predicted to be able to produce a high-energy component as well, but previous observations have not revealed such a signature clearly, probably due to the small number of >10 GeV photons even for the brightest GRBs known so far. In this Letter, we report on the Fermi Large Area Telescope (LAT) observations of the >100 MeV emission from the very bright and nearby GRB 130427A. We characterize the time-resolved spectra of the GeV emission from the GRB onset to the afterglow phase. Based on detection of about a dozen >10 GeV photons from GRB 130427A, we found a strong evidence of an extra hard spectral component that exists in the extended high-energy emission of this GRB. We argue that this hard component may arise from the afterglow inverse Compton emission.
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http://arxiv.org/abs/1305.3217
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