A wide dynamic range experiment to measure high energy γ-showers in air by detecting Cherenkov light in the middle ultraviolet
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G. Apollinari | G. Bellettini | G. Chiarelli | M. Dell'Orso | P. Giannetti | A. Menzione | L. Ristori | A. Scribano | S. Belforte | F. Bedeschi | F. Zetti | E. Bertolucci | A. Stefanini | P. Sestini | F. Cervelli
[1] A. Ciocio,et al. Observation of a time modulated muon flux in the direction of Cygnus X-3 , 1985 .
[2] Joyce,et al. Evidence for muon production by particles from Cygnus X-3. , 1985, Physical review letters.
[3] G. Chanmugam,et al. Ultra-high energy γ rays and cosmic rays from accreting degenerate stars , 1985, Nature.
[4] N. Porter. Astronomy: Ultra-high-energy γ rays from Cygnus X-3 , 1983, Nature.
[5] G. Charpak. Some recent trends in the evolution of gaseous detectors , 1982 .