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. 2020 Feb 14;7:10. doi: 10.1186/s40658-020-0275-6

Table 6.

Camera calibration factor and dead-time constant (± SE) derived from planar and threshold-segmented SPECT data with reduced wide-spectrum window width

Phantom 55–250 keV wide spectrum and TEW 55–229 keV wide spectrum and DEW
Calibration factor (cps/MBq) Dead-time constant (μs) Calibration factor (cps/MBq) Dead-time constant (μs)
Air-2Da 9.36 ± 0.01 0.632 ± 0.003 9.54 ± 0.01 0.534 ± 0.003
Air-3D 9.19 ± 0.05 0.638 ± 0.014 9.39 ± 0.05 0.565 ± 0.018
CTDI-10 9.30 ± 0.07 0.686 ± 0.019 9.48 ± 0.07 0.555 ± 0.021
CTDI-16 9.35 ± 0.08 0.606 ± 0.038 9.54 ± 0.08 0.462 ± 0.041
CTDI-32 9.31 ± 0.06 0.658 ± 0.020 9.44 ± 0.07 0.476 ± 0.026
Jaszczak 9.38 ± 0.05 0.673 ± 0.015 9.70 ± 0.06 0.496 ± 0.029

TEW: triple-energy window scatter correction. DEW: dual-energy windows scatter correction. Method B (full-range CF), with wide-spectrum acquisition count rate, was used to derive the calibration factor and the dead-time constant. aPlanar images of Air-2D phantom were not segmented, and data from both detectors was averaged