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Table 4 The \(\upgamma\) emissions used to calculate the intrinsic detector efficiency

From: Quantitative validation of Monte Carlo SPECT simulation: application to a Mediso AnyScan GATE simulation

Isotope

Energy (keV)

Intensity (%)

Activity (kBq)

\(^{210}\)Pb

46

4.25 ± 0.04

32.82 ± 0.34

\(^{241}\)Am

60

35.9 ± 0.4

276.2 ± 1.0

\(^{133}\)Ba

81

32.9 ± 0.3

129.30 ± 0.88

\(^{109}\)Cd

88

3.644 ± 0.016

75.54 ± 0.46

\(^{177}\)Lu

113

6.23 ± 0.04

512.3 ± 2.5

\(^{99\text {m}}\)Tc

140

89 ± 4

170.6 ± 1.5

\(^{123\text {m}}\)Te

159

84.0 ± 0.4

58.325± 0.085

\(^{139}\)Ce

166

79.90 ± 0.04

50.75 ± 0.51

\(^{177}\)Lu

208

10.41 ± 0.04

512.3 ± 2.5

\(^{133}\)Ba

356

62.05 ± 0.19

129.30 ± 0.88

  1. The quoted activities correspond to the start of the planar acquisition and standard uncertainties are given. \(\upgamma\) emission intensities are taken from [22]. Energy uncertainties are not given as they were significantly smaller than the energy resolution of the SPECT camera