Table 6: Best estimates for the pep and CNO solar neutrino interaction rates. For the results in the last two columns both statistical and systematic uncertainties are considered. Total fluxes have been obtained assuming MSWLMA and using the scattering crosssections from [146, 148, 149] and a scintillator density of . The last column gives the ratio between our measurement and the highZ (GS98) SSM [64]. Table taken from [74].  
