Abstract
The Very Energetic Radiation Imaging Telescope Array System (VERITAS) is an array of seven 10m aperture telescopes used for gamma-ray astronomy in the 50 GeV to 50 TeV (1 TeV= 1012 electron Volt) energy range. The gamma rays are detected by measuring the optical Cherenkov light emitted by the cascade of electromagnetic particles that is generated by interactions of the high energy gamma-ray with the Earth's Atmosphere. This paper describes the science goals of the VERITAS array, a description of the array, and expected performance of the instrument.
Original language | English (US) |
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Title of host publication | Proceedings of SPIE - The International Society for Optical Engineering |
Editors | P. Guhathakurta |
Pages | 276-287 |
Number of pages | 12 |
Volume | 4834 |
DOIs | |
State | Published - 2002 |
Event | Discoveries and Research Prospects from 6- to 10- Meter-Class telescopes II - Waikoloa, HI, United States Duration: Aug 22 2002 → Aug 23 2002 |
Other
Other | Discoveries and Research Prospects from 6- to 10- Meter-Class telescopes II |
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Country/Territory | United States |
City | Waikoloa, HI |
Period | 8/22/02 → 8/23/02 |
Keywords
- AGN
- Atmospheric Cherenkov radiation, Pulsars
- Cosmic rays
- Fundamental Physics
- Galactic Plane
- Gamma-ray Astronomy
- Gamma-ray telescopes
- Neutralinos
- Supernova remnants
- VERITAS