The Super-Kamiokande detector

By S. Fukuda, Y. Fukuda, T. Hayakawa, E. Ichihara, M. Ishitsuka, Y. Itow, T. Kajita, J. Kameda, K. Kaneyuki, S. Kasuga and 167 more. 2003

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Measurement of neutrino and antineutrino oscillations by the T2K experiment including a new additional sample of nu(e) interactions at the far detector (2017, unknown): “The T2K far detector is Super-Kamiokande [74], a 50 kt water Cherenkov detector located in the Kamioka Observatory, Gifu, Japan.”
OBSERVING THE NEXT GALACTIC SUPERNOVA (2013, background): “The Super–Kamiokande detector (Fukuda et al. 2003) in Japan has a nominal fiducial volume of 22.5 kton of ultra-pure water, and for a core collapse at the Milky Way center, Super–Kamiokande expects to detect Nνp ∼ 104 inverse beta events over several seconds, with a negligible number of background…”
Solar Neutrinos: Status and Prospects (2012, background): “…is shared between the scattered electron and outgoing neutrino, electron detection provides some sensitivity to the initial neutrino spectrum and thus to distortions associated with neutrino oscillations (Super-Kamiokande Collaboration 2012; Super-Kamiokande Collaboration, S. Fukuda et al. 2003).”
Hyper-Kamiokande (2020, methodology): “Hyper-Kamiokande is based on the proven technology of the highly successfull Super-Kamiokande detector [3].”
Theia: an advanced optical neutrino detector (2019, background): “1 ns [37]), and other performance characteristics are also much improved [36, 38].”