Current Status and Future Prospects of the SNO+ Experiment

Figure 9

True, reconstructed, and best fit SN neutrino energy distribution of the-p ES detection channel within the FV and above the detector threshold [16]. Shown is the sum of the,, andspectra, considering their time-integrated flux in the first second of the reference SN. The statistical uncertainties are shown in black, while the total uncertainties are shown in blue. The contribution from systematic uncertainty is too small to be resolved.