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Featured researches published by E. Pare.


Physics Letters B | 1990

Inclusive production of π0'S in the fragmentation region at the SppS collider

E. Pare; T. Doke; M. Haguenauer; V. Innocente; K. Kasahara; T. Kashiwagi; J. Kikuchi; S. Lanzano; Kimiaki Masuda; H. Murakami; Yasushi Muraki; T. Nakada; A. Nakamoto; T. Yuda

Abstract The inclusive production of π0s has been measured in the nucleon fragmentation region at the S p pS Collider at 630 GeV center of mass energy. Average transverse momentum and rapidity distributions compared with lower energy ISR data show no sizable violation of Feynman scaling in the fragmentation region.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1998

A NEW ANALYSIS METHOD FOR VERY HIGH DEFINITION IMAGING ATMOSPHERIC CHERENKOV TELESCOPES AS APPLIED TO THE CAT TELESCOPE

S. Le Bohec; B. Degrange; M. Punch; A. Barrau; R. Bazer-Bachi; H. Cabot; L.M. Chounet; G. Debiais; J. P. Dezalay; A. Djannati-Ataı̈; D. Dumora; P. Espigat; B. Fabre; P. Fleury; G. Fontaine; R. George; C. Ghesquiere; P. Goret; C. Gouiffes; I. A. Grenier; L. Iacoucci; I. Malet; C. Meynadier; F. Munz; T. Palfrey; E. Pare; Y. Pons; J. Quebert; K. Ragan; C. Renault

Abstract A new method of shower-image analysis is presented which appears very powerful as applied to those Cherenkov Imaging Telescopes with very high definition imaging capability. It provides hadron rejection on the basis of a single cut on the image shape, and simultaneously determines the energy of the electromagnetic shower and the position of the shower axis with respect to the detector. The source location is also reconstructed for each individual γ-ray shower, even with one single telescope, so for a point source the hadron rejection can be further improved. As an example, this new method is applied to data from the CAT (Cherenkov Array at Themis) imaging telescope, which has been operational since Autumn, 1996.


Physics Letters B | 1992

Searching for TeV dark matter by atmospheric Čerenkov techniques

M. Urban; A. Bouquet; B. Degrange; P. Fleury; J. Kaplan; A. L. Melchior; E. Pare

Abstract There is a growing interest in the possibility that dark matter could be formed of weakly interacting particles with a mass in the 100 GeV-2 TeV range, and supersymmetric particles are favorite candidates. If they constitute the dark halo of our Galaxy, their mutual annihilations produce energetic gamma rays that could be detected using existing atmospheric Cerenkov techniques.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2002

CELESTE: an atmospheric Cherenkov telescope for high energy gamma astrophysics

E. Pare; B. Balauge; R. Bazer-Bachi; H. Bergeret; F. Berny; N. Briand; Ph. Bruel; M. Cerutti; J. Collon; A. Cordier; P. Cornebise; G. Debiais; J.-P. Dezalay; D. Dumora; E. Durand; P. Eschstruth; P. Espigat; B. Fabre; P. Fleury; J. Gilly; J.-C. Gouillaud; C. Gregory; N. Hérault; J. Holder; M. Hrabovsky; S. Incerti; A. Jouenne; L. Kalt; R. LeGallou; B. Lott

Abstract 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 m 2 ) 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.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1989

Energy and position resolution of silicon calorimeter used in the UA7 experiment

J. Bourotte; M. Haguenauer; E. Pare; V. Innocente; S. Lanzano; K. Kasahara; Yasushi Muraki; T. Yuda; A. Nakamoto; H. Murakami; T. Doke; T. Kashiwagi; J. Kikuchi; Kimiaki Masuda

Abstract The performance of a compact 4 in. diameter, 20 radiation lengths silicon/tungsten calorimeter has been evaluated using electron and pion beams up to 100 GeV at the CERN SPS. The energy and position resolutions have been found to be respectively ( 25% √E + 1.1%) GeV and 3.8 mm /√E .


Astronomy and Astrophysics | 1999

Very high-energy gamma-ray spectral properties of Mrk 501 from cat Cherenkov telescope observations in 1997

A. Djannati-Ataï; F. Piron; Aurelien Barrau; L. Iacoucci; M. Punch; J-P. Tavernet; R. Bazer-Bachi; H. Cabot; L.-M. Chounet; G. Debiais; B. Degrange; J-P. Dezalay; D. Dumora; P. Espigat; B. Fabre; Pascal Fleury; G. Fontaine; C. Ghesquiere; P. Goret; C. Gouiffes; I-A. Grenier; S. Le Bohec; I. Malet; C. Meynadier; G. Mohanty; E. Nuss; E. Pare; J. Quebert; K. Ragan; C. Renault


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1998

Prototype tests for the CELESTE solar array gamma-ray telescope

B. Giebels; R. Bazer-Bachi; H. Bergeret; A. Cordier; G. Debiais; M. DeNaurois; J. P. Dezalay; D. Dumora; P. Eschstruth; P. Espigat; B. Fabre; P. Fleury; C. Ghesquiere; N. Herault; I. Malet; B. Merkel; C. Meynadier; M. Palatka; E. Pare; J. Procureur; M. Punch; J. Quebert; K. Ragan; L. Rob; P. Schovanek; D. Smith; J. Vrana


arXiv: Astrophysics | 1997

Performances of the CAT imaging telescope and some preliminary results on Mkn 180 and the Crab

A. Barrau; R. Bazer-Bachi; H. Cabot; L.-M. Chounet; G. Debiais; B. Degrange; J. P. Dezalay; A. Djannati-Atai; D. Dumora; P. Espigat; B. Fabre; P. Fleury; G. Fontaine; R. George; C. Ghesquiere; P. Goret; C. Gouiffes; I. A. Grenier; L. Iacoucci; S. Le Bohec; I. Malet; C. Meynadier; P. Munz; T. Palfrey; E. Pare; Y. Pons; M. Punch; J. Quebert; K. Ragan; C. Renault


arXiv: Astrophysics | 1997

Detection of Vhe Gamma-Rays from MRK 501 with the Cat Imaging Telescope

Aurelien Barrau; R. Bazer-Bachi; H. Cabot; L.-M. Chounet; G. Debiais; B. Degrange; J-P. Dezalay; A. Djannati-Ataï; D. Dumora; P. Espigat; B. Fabre; Pascal Fleury; G. Fontaine; R. George; C. Ghesquiere; P. Goret; C. Gouiffes; I-A. Grenier; L. Iacoucci; S. Le Bohec; I. Mallet; C. Meynadier; F. Munz; T. Palfrey; E. Pare; Y. Pons; M. Punch; J. Quebert; K. Ragan; C. Renault


arXiv: Astrophysics | 1997

Observation of the Crab Nebula Gamma-Ray Emission Above 220 Gev by the Cat Cherenkov Imaging Telescope

A. Barrau; R. Bazer-Bachi; H. Cabot; L.-M. Chounet; G. Debiais; B. Degrange; J. P. Dezalay; A. Djannati-Atai; D. Dumora; P. Espigat; B. Fabre; P. Fleury; G. Fontaine; R. George; C. Ghesquiere; P. Goret; C. Gouiffes; I. A. Grenier; L. Iacoucci; S. Le Bohec; I. Mallet; C. Meynadier; F. Munz; T. Palfrey; E. Pare; Y. Pons; M. Punch; J. Quebert; K. Ragan; C. Renault

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B. Fabre

University of Perpignan

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R. Bazer-Bachi

Centre national de la recherche scientifique

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C. Meynadier

University of Perpignan

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H. Cabot

University of Perpignan

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