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Kamiokande, associated with Masatoshi Koshiba, was an underground water Cherenkov detector viewed by photomultipliers. Improved water purity and reduced background enabled solar neutrino observations. A concentration of reconstructed recoil directions toward the Sun distinguished a source signal above an approximately direction-independent background.^[ref]

For solar neutrinos, electron elastic scattering supplies a directional recoil, with different cross sections for active neutrino flavors. Neither the Homestake experiment deficit nor the SN 1987A neutrino burst alone established neutrino oscillation; later evidence compared complementary channels and propagation effects.^[ref]

Masatoshi Koshiba helped turn underground neutrino detectors into astronomical instruments. The Kamiokande II report of the 1987 supernova burst described eleven electron-like events over about thirteen seconds. These rare interactions supplied information about the collapsing star through weakly interacting particles rather than only its escaping light. The observation joined the timing and energy measurements of particle detection with a transient event far outside the solar system.^[ref]

A physicist.^[ref]

One quarter each went to Raymond Davis Jr. and Masatoshi Koshiba for pioneering astrophysics through detection of cosmic neutrinos. One half went to Riccardo Giacconi for pioneering astrophysics leading to the discovery of cosmic X-ray sources.^[ref]