Orateur
Sylvia Zhu
(DESY)
Description
In the last few years, very-high-energy (>100 GeV) emission from gamma-ray bursts (GRBs) has been detected for the first time, allowing us to build a multiwavelength picture of GRBs that extends all the way up to TeV energies. Now that we’ve detected a few GRBs, the question becomes: What’s next? In this talk, I will describe the GRB programs of the current generation of air Cherenkov telescopes and the context in the multiwavelength community.
