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Operating performance of the gamma-ray Cherenkov telescope: An end-to-end Schwarzschild–Couder telescope prototype for the Cherenkov Telescope Array

Abstract:

The Cherenkov Telescope Array (CTA) consortium aims to build the next-generation ground-based very-high-energy gamma-ray observatory. The array will feature different sizes of telescopes allowing it to cover a wide gamma-ray energy band from about 20 GeV to above 100 TeV. The highest energies, above 5 TeV, will be covered by a large number of Small-Sized Telescopes (SSTs) with a field-of-view of around 9°. The Gamma-ray Cherenkov Telescope (GCT), based on Schwarzschild–Couder dual-mirror opti...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1016/j.nima.2016.05.059

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
Publisher:
Elsevier
Journal:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment More from this journal
Volume:
845
Pages:
355-358
Publication date:
2016-05-01
Acceptance date:
2016-05-14
DOI:
EISSN:
1872-9576
ISSN:
0168-9002
Keywords:
Pubs id:
pubs:629374
UUID:
uuid:d5e6dfe5-d1cb-48a8-970b-03c075f7fe59
Local pid:
pubs:629374
Source identifiers:
629374
Deposit date:
2018-02-03

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