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Extending the Sensitivity of Air Cerenkov Telescopes

Abstract:

Over the last decade, the Imaging Air Cerenkov technique has proven itself to be an extremely powerful means to study very energetic gamma-radiation from a number of astrophysical sources in a regime which is not practically accessible to satellite-based instruments. The further development of this approach in recent years has generally concentrated on increasing the density of camera pixels, increasing the mirror area and using multiple telescopes. Here we present a practical method to subst...

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Publication status:
Published

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Authors


Perez, IDLC More by this author
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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Particle Physics
Journal:
Astropart.Phys.
Volume:
26
Issue:
2
Pages:
69-90
Publication date:
2006-02-13
DOI:
ISSN:
0927-6505
URN:
uuid:5cdbd2d7-95bb-4d8a-8b99-0bd79859aa3b
Source identifiers:
28416
Local pid:
pubs:28416
Language:
English
Keywords:

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