VERITAS: Very LArge Energetic Radiation Imaging Telescope Array System
Weekes, T. C. · Akerlof, C. · Biller, S. · Breslin, A. C. · Buckley, J. H. · Carter-Lewis, D. A. · Catanese, M. · Cawley, M. F. · Dingus, B. · Fazio, G. G. · Fegan, D. J. · Finley, J. · Fishman, G. · Gaidos, J. · Gillanders, G. H. · Gorham, P. · Grindlay, J. E. · Hillas, A. M. · Huchra, J. · Kaaret, P. · Kertzman, M. · Kieda, D. · Krennrich, F. · Lamb, R. C. · Lang, M. J. · Marscher, A. P. · Matz, S. · McKay, T. · Muller, D. · Ong, R. · Purcell, W. · Rose, J. · Sembroski, G. · Seward, F. D. · Slane, P. · Swordy, S. · Tumer, T. · Ulmer, M. · Urban, M. · Wilkes, B. J.
Original · EN
A next generation atmospheric Cherenkov observatory is described based on the Whipple Observatory γ-ray telescope. A total of nine such imaging telescopes will be deployed in an array that will permit the maximum versatility and give high sensitivity in the 50 GeV - 50 TeV band (with maximum sensitivity from 100 GeV to 10 TeV).
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