Gamma-ray burst observations with new generation imaging atmospheric Cerenkov Telescopes in the FERMI era

Details Gamma-ray burst observations with new generation imaging atmospheric Cerenkov Telescopes in the FERMI era Gamma-ray burst observations with new generation imaging atmospheric Cerenkov Telescopes in the FERMI era

2009-01-12

arxiv.org/abs/0901.1589v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

9 pages, two figures. Proceeding for the 6th "Science with the New Generation of High Energy Gamma-Ray Experiments" workshop

Scientific paper

10.1063/1.3125779

After the launch and successful beginning of operations of the FERMI satellite, the topics related to high-energy observations of gamma-ray bursts have obtained a considerable attention by the scientific community. Undoubtedly, the diagnostic power of high-energy observations in constraining the emission processes and the physical conditions of gamma-ray burst is relevant. We briefly discuss how gamma-ray burst observations with ground-based imaging array Cerenkov telescopes, in the GeV-TeV range, can compete and cooperate with FERMI observations, in the MeV-GeV range, to allow researchers to obtain a more detailed and complete picture of the prompt and afterglow phases of gamma-ray bursts.

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