VERITAS, an Imaging Atmospheric Cherenkov Telescope (IACT) system for gammma-ray astronomy in the GeV-TeV range, has recently completed its first season of observations with a full array of four telescopes. A number of astrophysical gamma-ray sources have been detected, both galactic and extragalactic, including sources previously unknown at TeV energies. We describe the status of the array and some highlight results, and assess the technical performance, sensitivity and shower reconstruction capabilities.

Status of the VERITAS Observatory

Cesarini, Andrea;
2009-01-01

Abstract

VERITAS, an Imaging Atmospheric Cherenkov Telescope (IACT) system for gammma-ray astronomy in the GeV-TeV range, has recently completed its first season of observations with a full array of four telescopes. A number of astrophysical gamma-ray sources have been detected, both galactic and extragalactic, including sources previously unknown at TeV energies. We describe the status of the array and some highlight results, and assess the technical performance, sensitivity and shower reconstruction capabilities.
2009
HIGH ENERGY GAMMA‐RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma‐Ray Astronomy
Heidelberg, Germany
American Institute of Physics
9780735406162
Cesarini, Andrea; Veritas, Collaboration
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11572/67591
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