Affiliation:
1. Dublin Institute for Advanced Studies, Dublin, Ireland.
2. Max Planck Institut fur Kernphysik, Heidelberg, Germany.
Abstract
Over the past few years, very-high-energy gamma-ray astronomy has emerged as a truly observational discipline, with many detected sources representing different galactic and extragalactic source populations—supernova remnants, pulsar wind nebulae, giant molecular clouds, star formation regions, compact binary systems, and active galactic nuclei. It is expected that observations with the next generation of stereoscopic arrays of imaging atmospheric Cherenkov telescopes over a very broad energy range from 10
10
to 10
15
electron volts will dramatically increase the number of very-high-energy gamma-ray sources, thus having a huge impact on the development of astrophysics, cosmology, and particle astrophysics.
Publisher
American Association for the Advancement of Science (AAAS)
Cited by
14 articles.
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