TenTen: A New Array of Multi-TeV Imaging Cherenkov Telescopes
| dc.creator | Rowell, G. | |
| dc.creator | Stamatescu, V. | |
| dc.creator | Clay, R. | |
| dc.creator | Dawson, B. | |
| dc.creator | Denman, J. | |
| dc.creator | Protheroe, R. | |
| dc.creator | Smith, A. G. K. | |
| dc.creator | Thornton, G. | |
| dc.creator | Wild, N. | |
| dc.date | 2007-10-10 | |
| dc.date.accessioned | 2026-07-07T08:35:27Z | |
| dc.date.available | 2026-07-07T08:35:27Z | |
| dc.description | 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. | |
| dc.description | 4 pages, 2 figures, proceedings of the 30th ICRC, Merida, Mexico, 2007 | |
| dc.identifier | https://arxiv.org/abs/0710.2027 | |
| dc.identifier | http://arxiv.org/abs/0710.2027 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/139755 | |
| dc.subject | Astrophysics | |
| dc.title | TenTen: A New Array of Multi-TeV Imaging Cherenkov Telescopes | |
| dc.type | text |