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. Author manuscript; available in PMC: 2022 Apr 1.
Published in final edited form as: Appl Radiat Isot. 2020 Dec 31;170:109572. doi: 10.1016/j.apradiso.2020.109572

Table 8.

Uncertainty budgets for the absolute emission intensity for the 241 keV γ-ray, Iγ, determined at NIST with the x-detector and at NPL using the S3 solution.

NPL
NIST
LET + HET GENIE LET + HET



/% /% /%
Standard uncertainty of weighted mean 0.11
Peak fitting and counting statistics 0.41 0.22 0.21
Source activity 0.27 0.31 0.31
Full-energy peak detection efficiency 0.34 0.71 0.71
Decay correction during measurement (NPL combined this component with “Decay factor to reference time” for a single component) 0.037 0.037
Decay factor to reference time 0.069 0.066 0.066
Dead time/Pile-up 0.1 0.006 0.006
Self-absorption (wholly embodied in NIST “Full-energy peak detection efficiency”) 0.065
Stability (wholly embodied in NIST “Full-energy peak detection efficiency”) 0.1
Gravimetric (wholly embodied in NIST “Source activity”) 0.02
228Th impurity <0.001 0.004 0.004

Combined standard uncertainty, uc 0.63 0.8 0.8
uc using correlation calculation from the GUM 0.59 0.59