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[en] The anisotropy of the positrons emitted in the reaction ν-bare + p → n + e+ has to be taken into account for extracting an antineutrino signal in Superkamiokande. For the Sun, this effect allows a sensitivity to νe → ν-bare transition probability at the 3% level already with the statistics collected in the first hundred days. For a supernova in the Galaxy, the effect is crucial for extracting the correct ratio of ν - e to ν-bare - p events
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