Prospects for Very High Energy γ-RAY Astronomy with Next Generation Imaging ČERENKOV Telescope

Details Prospects for Very High Energy γ-RAY Astronomy with Next Generation Imaging ČERENKOV Telescope Prospects for Very High Energy γ-RAY Astronomy with Next Generation Imaging ČERENKOV Telescope

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003omeg.conf...31k&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2000. Proceedings of the International Symposium. Held 19-21 January 2000 in Universi

Astronomy and Astrophysics

Astronomy

Scientific paper

The ground-based technique has opened a way of detecting γ-rays at ~1 TeV energy by collecting the energetic photons with detection area ~ 104m2 and angular resolution ~ 0.1°. The next step of improving sensitivity is now going to be taken to exploit, to a larger extent, violent energetic phenomena in which the process of particle acceleration plays a dominant role. The basic concept of the currently going-on projects for the next generation γ-ray telescope is described in this paper, paying an attention on how and why the current status of very high energy γ-ray astronomy needs to be developed for improvements.

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