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. 2022 Mar 8;13:818463. doi: 10.3389/fphys.2022.818463

Table 2.

Calculated recovery coefficient and contrast recovery and background noise for the images of NEMA IQ phantom for different image reconstruction and radionuclide combinations.

Sphere size Radionuclide Recovery coefficient Contrast recovery [%]
OSEM PRC Relative difference [%] OSEM PRC
10 mm 18F 0.54 0.53 −2.34 42.8 41.2
68Ga 0.37 0.49 32.51 28.4 42.2
124I 0.39 0.53 36.52 23.8 41.6
13 mm 18F 0.62 0.61 −1.8 52.5 51.1
68Ga 0.56 0.68 21.5 49.3 63.0
124I 0.50 0.63 25.0 38.1 53.9
17 mm 18F 0.73 0.72 −1.8 66.6 64.9
68Ga 0.61 0.68 10.1 55.8 62.9
124I 0.64 0.73 15.4 54.5 66.8
22 mm 18F 0.82 0.80 −1.7 77.2 75.5
68Ga 0.67 0.73 7.7 62.7 68.6
124I 0.75 0.81 8.2 68.8 76.5
28 mm 18F 0.84 0.81 −2.9 79.6 76.6
68Ga 0.72 0.79 8.7 68.5 75.8
124I 0.77 0.83 7.8 71.5 79.1
37 mm 18F 0.87 0.85 −1.8 83.9 81.9
68Ga 0.78 0.82 5.5 75.1 80.0
124I 0.85 0.88 4.4 80.7 85.3
Background noise [%]
18F 10.1 9.30 −8.3
68Ga 17.7 15.7 −11.0
124I 9.7 9.35 −3.8

18F images (both OSEM and PRC) were reconstructed with 3 iterations and 12 subsets, while 68Ga and 124I images with 2 iterations and 12 subsets for OSEM and 8 iterations as 12 subsets for PRC.