%0 Conference Proceedings
%T NECTAR: New Electronics for the Cherenkov Telescope Array
%+ Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE)
%+ Laboratoire de Physique Subatomique et de Cosmologie (LPSC)
%+ Laboratoire Univers et Particules de Montpellier (LUPM)
%A Naumann, C.L.
%A Bolmont, J.
%A Corona, P.
%A Delagnes, E.
%A Dzahini, Daniel
%A Feinstein, F.
%A Gascon, D.
%A Glicenstein, J.-F.
%A Nayman, P.
%A Rarbi, F.
%A Ribó, M.
%A Sanuy, A.
%A Sieiro, J.
%A Tavernet, J.-P.
%A Toussenel, F.
%A Vincent, P.
%A Vorobiov, S.
%< avec comité de lecture
%Z LPSC12366
%( PoS - Proceedings of Science
%B International Workshop on New Photon-Detectors (PhotoDet 2012)
%C Orsay, France
%V PoS(PhotoDet 2012)030
%P 030
%8 2012-06-13
%D 2012
%Z Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Conference papers
%X CTA is the next-generation Cherenkov Telescope Array currently under development by the international CTA consortium, based on experience from the three major telescope arrays of the current generation, H.E.S.S., MAGIC and VERITAS. A new kind of front-end hardware, both powerful and flexible, yet inexpensive, will be required to achieve a sensitivity and energy range which is hitherto unprecedented for TeV gamma rays. One possible solution to equip the up to 100 planned telescopes (with a total of around 100000 photodetector channels) while providing a high degree of flexibility for both triggering and telescope readout is offered by the NECTAr system (New Electronics for the Cherenkov Telescope Array), integrating as much of the front-end functionality as possible into a single ASIC (including pre-amplifiers, fast analog samplers, memory and ADCs). The current status of its development, together with results from measurements and simulations are presented
%G English
%L in2p3-00805284
%U https://hal.in2p3.fr/in2p3-00805284
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