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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. Ghesquière,N. Herault,I. Malet,B. Merkel,C. Meynadier,M. Palatka,E. Paré,J. Procureur,M. Punch,J. Québert,K. Ragan,L. Rob,P. Schovanek,D.A. Smith,J. Vrana

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment（1998）

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摘要
The CELESTE experiment will be an atmospheric Cherenkov detector designed to bridge the gap in energy sensitivity between current satellite and ground-based gamma-ray telescopes, 20–300GeV. We present test results made at the former solar power plant, Themis, in the French Pyrenees. The tests confirm the viability of using a central tower heliostat array for Cherenkov wavefront sampling.
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gamma ray
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