Abstract
Gamma-ray bursts have been detected at photon energies up to tens of GeV. We review some recent developments in the X-ray to GeV photon phenomenology in the light of Swift and Fermi observations, and some of the theoretical models developed to explain them, with a view towards implications for C.T.A.
Original language | English (US) |
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Pages (from-to) | 134-141 |
Number of pages | 8 |
Journal | Astroparticle Physics |
Volume | 43 |
DOIs | |
State | Published - 2013 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics