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Pare, E.; Balauge, B.; Bazer-Bachi, R.; Bergeret, H.; Berny, F.; Briand, N.; Bruel, P.; Cerutti, M.; Collon, J.; Cordier, A.; Cornebise, P.; Debiais, G.; Dezalay, J.-P.; Dumora, D.; Durand, E.; Eschstruth, P.; Espigat, P.; Fabre, B.; Fleury, P.; Gilly, J.; Gouillaud, J.-C.; Gregory, C.; Herault, N.; Holder, J.; Hrabovsky, M.; Incerti, S.; Jouenne, A.; Kalt, L.; LeGallou, R.; Lott, B.; Lodygensky, O.; Manigot, P.; Manseri, H.; Manitaz, H.; Martin, M.; Morano, R.; Morineaud, G.; Muenz, F.; Musquere, A.; Naurois, M. de; Neveu, J.; Noppe, J.-M.; Olive, J.-F.; Palatka, M.; Perez, A.; Quebert, J.; Rebii, A.; Reposeur, T.; Rob, L.; Roy, P.; Sans, J.-L.; Sako, T.; Schovanek, P.; Smith, D.A.; Snabre, P.; Villard, G., E-mail: reposeur@in2p3.fr2002
AbstractAbstract
[en] CELESTE is an atmospheric Cherenkov telescope based on the sampling method which makes use of the de-commissioned THEMIS solar electrical plant in the French Pyrenees. A large (2000 m2) mirror surface area from 40 independent heliostats followed by a secondary optic, a trigger system using analog summing techniques and signal digitization with 1 GHz flash ADCs make possible the detection of cosmic γ-rays down to 30 GeV. This paper provides a detailed technical description of the CELESTE installation
Primary Subject
Source
S0168900202010057; Copyright (c) 2002 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA)
Record Type
Journal Article
Journal
Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment; ISSN 0168-9002; ; CODEN NIMAER; v. 490(1-2); p. 71-89
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INIS VolumeINIS Volume
INIS IssueINIS Issue