N. Fouque
University of Savoy
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Featured researches published by N. Fouque.
arXiv: Instrumentation and Methods for Astrophysics | 2016
J. F. Glicenstein; O. Abril; J-A. Barrio; O. Blanch Bigas; J. Bolmont; F. Bouyjou; P. Brun; E. Chabanne; C. Champion; S. Colonges; P. Corona; E. Delagnes; C. Delgado; C. Diaz Ginzov; D. Durand; J.-P. Ernenwein; S. J. Fegan; O. Ferreira; M. Fesquet; A. Fiasson; G. Fontaine; N. Fouque; D. Gascon; B. Giebels; François Hénault; R. Hermel; D. Hoffmann; D. Horan; J. Houles; P. Jean
NectarCAM is a camera proposed for the medium-sized telescopes of the Cherenkov Telescope Array (CTA) covering the central energy range of ~100 GeV to ~30 TeV. It has a modular design and is based on the NECTAr chip, at the heart of which is a GHz sampling Switched Capacitor Array and a 12-bit Analog to Digital converter. The camera will be equipped with 265 7-photomultiplier modules, covering a field of view of 8 degrees. Each module includes the photomultiplier bases, high voltage supply, pre-amplifier, trigger, readout and Ethernet transceiver. The recorded events last between a few nanoseconds and tens of nanoseconds. The camera trigger will be flexible so as to minimize the read-out dead-time of the NECTAr chips. NectarCAM is designed to sustain a data rate of more than 4 kHz with less than 5% dead time. The camera concept, the design and tests of the various subcomponents and results of thermal and electrical prototypes are presented. The design includes the mechanical structure, cooling of the electronics, read-out, clock distribution, slow control, data-acquisition, triggering, monitoring and services.
Proceedings of the Tenth International Conference | 2003
R. Kossakowski; F. Cadoux; V. Chambert-Hermel; G. Coignet; J.M. Dubois; D. Fougeron; N. Fouque; L. Girard; C. Goy; R. Hermel; B. Lieunard; S. Rosier-Lees; J.P. Vialle; G. Chen; H. S. Chen; Z. Liu; Y. Lu; Z. Yu; H.L. Zhuang; F. Cervelli; S. Di Falco; T. Lomtadze; G. Venanzoni; E. Falchini; P. Maestro; P.S. Marrocchesi; R. Paoletti; F. Pilo; N. Turini; G. Valle
The electromagnetic calorimeter (ECAL) of the AMS-02 experiment is a 3-dimensional sampling calorimeter, made of lead and scintillating fibers. The detector allows for a high granularity, with 18 samplings in the longitudinal direction, and 72 sampling in the lateral direction. The ECAL primary goal is to measure the energy of cosmic rays up to few TeV, however, thanks to the fine grained structure, it can also provide the separation of positrons from protons, in the GeV to TeV region. A direct measurement of high energy photons with accurate energy and direction determination can also be provided.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2013
C. Adloff; L. Basara; G. Bigongiari; F. Bosi; P. Brun; F. Cadoux; F. Cervelli; V. Chambert; G. Chen; Gen Chen; H. S. Chen; G. Coignet; G. Cougoulat; S. Di Falco; J.M. Dubois; S. Elles; E. Falchini; A. Fiasson; D. Fougeron; N. Fouque; S. Galeotti; G. Gallucci; F. Gherarducci; L. Girard; F. Giuseppe; C. Goy; R. Hermel; M. Incagli; J. Jacquemier; L. Journet
arXiv: Instrumentation and Methods for Astrophysics | 2013
J. F. Glicenstein; M. Barceló; J-A. Barrio; O. Blanch; J. Boix; J. Bolmont; C. Boutonnet; S. Cazaux; E. Chabanne; C. Champion; Frederic Chateau; S. Colonges; P. Corona; S. Couturier; B. Courty; E. Delagnes; C. Delgado; J.-P. Ernenwein; S. J. Fegan; O. Ferreira; M. Fesquet; G. Fontaine; N. Fouque; François Hénault; D. Gascon; D. Herranz; R. Hermel; D. Hoffmann; J. Houles; S. Karkar
International Conference on Calorimetry in Particle Physics 10 CALOR 2002 | 2002
R. Kossakowski; F. Cadoux; V. Chambert-Hermel; G. Coignet; J.M. Dubois; D. Fougeron; N. Fouque; L. Girard; C. Goy; R. Hermel; B. Lieunard; S. Rosier-Lees; J.P. Vialle; G. Chen; H. S. Chen; Z. Liu; Y. Lu; Z. Yu; H.L. Zhuang; F. Cervelli; S. Di Falco; T. Lomtadze; G. Venanzoni; E. Falchini; P. Maestro; P.S. Marrocchesi; R. Paolietti; F. Pilo; N. Turini; G. Valle