TenTen: A New Array of Multi-TeV Imaging Cherenkov Telescopes
G. Rowell, V. Stamatescu, R. Clay, B. Dawson, J. Denman, R. Protheroe,, A.G.K. Smith, G. Thornton, N. Wild

TL;DR
TenTen is a proposed array of Cherenkov telescopes designed to explore the multi-TeV gamma-ray energy range, aiming to discover new astrophysical sources and study cosmic-ray origins with a large effective area.
Contribution
This paper introduces the TenTen array, a novel Cherenkov telescope system optimized for multi-TeV gamma-ray observations, with detailed performance parameters.
Findings
Effective area of ~10 km^2 above 10 TeV
Wide field of view of 8-10 degrees
Optimized for energies between 10 and 100 TeV
Abstract
The exciting results from H.E.S.S. point to a new population of gamma-ray sources at energies E > 10 TeV, paving the way for future studies and new discoveries in the multi-TeV energy range. Connected with these energies is the search for sources of PeV cosmic-rays (CRs) and the study of multi-TeV gamma-ray production in a growing number of astrophysical environments. TenTen is a proposed stereoscopic array (with a suggested site in Australia) of modest-sized (10 to 30m^2) Cherenkov imaging telescopes with a wide field of view (8 to 10deg diameter) optimised for the E~10 to 100 TeV range. TenTen will achieve an effective area of ~10 km^2 at energies above 10 TeV. We outline here the motivation for TenTen and summarise key performance parameters.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Particle Detector Development and Performance · Dark Matter and Cosmic Phenomena
