Solar neutrino precision measurements using all 1496 days of Super-Kamiokande-I data

The results of the entire Super-Kamiokande-1 solar neutrino data are presented. The measured interaction rate is 47±2% of the rate expected by the standard solar model and 133±5% of the rate implied by the SNO charged-current interaction rate. There is no evidence for spectral distortion or a time dependent neutrino flux. Together with the rates of other experiments, the Super-Kamiokande results imply active solar neutrino oscillations and restrict neutrino mixing and mass square difference to lie within the LMA solution area