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. 2019 Apr 29;46(6):2690–2695. doi: 10.1002/mp.13536

Table 1.

Photon energy, location of Gaussian fit, and calculated energy resolution

Isotope Photon energy (keV) Gaussian fit center (keV) FWHM/E0 ± SD
99mTc 141 142 ± 1.3 67% ± 1.3%
133Ba 344 340 ± 1.9 67% ± 2.6%
18F 511 515 ± 4.4 42% ± 3.2%
137Cs 662 666 ± 5.6 32% ± 4.2%

Note that the photon energy used for 133Ba is a weighted average of the three photon emissions near the most abundant (356 keV).