The VERITAS Atmospheric Cerenkov Telescopes: Positioner, Optics and Associated Components

Details The VERITAS Atmospheric Cerenkov Telescopes: Positioner, Optics and Associated Components The VERITAS Atmospheric Cerenkov Telescopes: Positioner, Optics and Associated Components

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....5.2823g&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

1

Scientific paper

The Very Energetic Radiation Imaging telescope Array System (VERITAS)[1,2] is a next generation ground-based TeV gamma-ray detector. VERIˇ TAS will consist of seven 12 m aperture atmospheric Cerenkov telescopes. The design of these telescopes builds on three decades of experience with the Whipple 10-m. Significant improvements have been made in their optical and tracking performance, and hence, in their ability to exploit the VERITAS high-resolution cameras and stereo imaging capability.

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