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Abundance of primary protons at (1–3)× eV inferred from a simulation of extensive air showers with γ-ray families
National licenceAmerican Physical Society | 1989| -
Inelastic -Air Cross Section at Energies between and eV Estimated from Air-Shower Experiments
National licenceAmerican Physical Society | 1983| -
Atmospheric gamma-ray observation with the BETS detector for calibrating atmospheric neutrino flux calculations
National licenceAmerican Physical Society | 2002| -
Extensive air showers accompanied by γ-ray families with J,H≥10 TeV and general extensive air showers
National licenceAmerican Physical Society | 1989| -
Nuclear interactions and primary cosmic-ray component around eV viewed through the cluster analysis of -ray families
National licenceAmerican Physical Society | 1982| -
Hadronic interactions at energies around TeV inferred from the large-scale emulsion-chamber experiment at Mt. Fuji
National licenceAmerican Physical Society | 1981| -
Hadronic interactions and primary-cosmic-ray composition at energies around – eV derived from the analysis of high-energy gamma families
National licenceAmerican Physical Society | 1988| -
Properties of hadron families observed with thick-type emulsion chambers at Mts. Kanbala and Fuji and search for Centauro events
National licenceAmerican Physical Society | 1988| -
Primary-cosmic-ray protons above eV derived from the observation of superhigh-energy halo events
National licenceAmerican Physical Society | 1988| -
Search for γ rays from the supernova 1987A at energies greater than 100 TeV
National licenceAmerican Physical Society | 1988| -
Search for TeV rays from SN 1987 A during December 1987 and January 1988
National licenceAmerican Physical Society | 1988| -
Search for point sources of ultrahigh energy rays in the southern sky
National licenceAmerican Physical Society | 1993| -
Cosmic-ray deficit from the directions of the Moon and the Sun detected with the Tibet air-shower array
National licenceAmerican Physical Society | 1993| -
Search for steady emission of 10-TeV gamma rays from the Crab Nebula, Cygnus X-3, and Hercules X-1 using the Tibet air shower array
National licenceAmerican Physical Society | 1992| -
Measurement of air shower cores to study the cosmic ray composition in the knee energy region
National licenceAmerican Physical Society | 2000| -
Primary proton spectrum between 200 TeV and 1000 TeV observed with the Tibet burst detector and air shower array
National licenceAmerican Physical Society | 2000|
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