Measurement of the B 8 solar neutrino flux using the full SNO + water phase dataset
The SNO+ detector operated initially as a water Cherenkov detector. The implementation of a sealed cover gas system midway through water data taking resulted in a significant reduction in the activity of 222 Rn daughters in the detector and allowed the lowest background to the solar electron scattering signal above 5 MeV achieved to date. This paper reports an updated SNO+ water phase 8 B solar neutrino analysis with a total livetime of 282.4 days and an analysis threshold of 3.5 MeV. The 8 B solar neutrino flux is found to be (2.32$^{+0.18}_{-0.17}$(stat)$^{+0.07}_{-0.05}$(syst))×10 6 cm -2 s -1 assuming no neutrino oscillations, or (5.36$^{+0.41}_{-0.39}$(stat)+$^{0.17}_{-0.16}$(syst))×10 6 cm -2 s -1 assuming standard neutrino oscillation parameters, in good agreement with both previous measurements and standard solar model calculations. The electron recoil spectrum is presented above 3.5 MeV.