Toru Tanimori

TL;DR: The ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes as mentioned in this paper, which is an international initiative to build the next generation instrument, with a factor of 5-10 improvement in sensitivity in the 100 GeV-10 TeV range and the extension to energies well below 100GeV and above 100 TeV.

TL;DR: In this article, the authors presented results from 1036 days of solar neutrino data accumulated in the upgraded Kamiokande detector (KAMIOKande III) and showed that no strong correlation of the solar NE flux with the sunspot numbers was found within experimental errors.

TL;DR: In this article, the Kamiokande detector was used to study the atmospheric (v μ + v μ ) (v e + v e ) ratio in the multi-GeV energy range.

TL;DR: In this paper, the Kamiokande detector was used to observe atmospheric neutrino interactions in an exposure of 4.92 kt yr and the observed ratio of single ring μ-events to e-events (μ e ) data ( μ e ) MC = 0.60 +007 −0.06 ( stat. ) ± 0.05 ( syst. ) suggests that the atmospheric vμ/ve ratio is smaller than expected.

TL;DR: In this paper, the number of electron-like single-prong events is in good agreement with the predictions of a Monte Carlo calculation based on atmospheric neutrino interactions in the KAMIOKANDE detector.