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Figure 10: The neutrino-induced electron recoil spectra expected in Borexino. The total rates are those predicted by the latest high-Z solar model [64]. The pep and CNO neutrinos recoil spectra with end points in the region 1.2–1.5 MeV are shown. Also the Be neutrinos (measured in [129]), with a count rate about 10 times larger, are shown for comparison. Note that the variable on the -axis is not directly the energy value. Taken from [131].