“…Applying the offline correction factors to the peaks revealed the following energies with an uncertainty of ±7.5 keV: 1,277, 1,003, 877, 729, and 595 keV. The most probable emissions between 511 keV and 1.3 MeV for 154 Eu are 1,274.4, 1,004.7, 996.3, 873.2, 723.3, and 591.8 keV [ 13 , 14 , 15 ]. The agreement of the measured values to within 1% of the expected energies supports our theory that the increased count rates and observed spectra are the result of 154 Eu emissions.…”