2010
DOI: 10.4103/0971-6203.71765
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Experimental determination of the weighting factor for the energy window subtraction-based downscatter correction for I-123 in brain SPECT studies

Abstract: Correction for downscatter in I-123 SPECT can be performed by the subtraction of a secondary energy window from the main window, as in the triple-energy window method. This is potentially noise sensitive. For studies with limited amount of counts (e.g. dynamic studies), a broad subtraction window with identical width is preferred. This secondary window needs to be weighted with a factor higher than one, due to a broad backscatter peak from high-energy photons appearing at 172 keV. Spatial dependency and the nu… Show more

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Cited by 13 publications
(12 citation statements)
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“…This point was addressed by investigating the relevance of extra-brain activity which is not accounted for in a phantom study. The high uptake and retention of [ 123 I]FP-CIT in lungs, liver, and intestines and sometimes in salivary glands and thyroid [ 9 ] is, in fact, expected to contribute to the brain image, particularly through septal penetration from the 123 I high-energy gamma emissions [ 10 , 11 ]. The magnitude of this contribution was indirectly estimated from a comparison of the phantom (brain activity only) and the human (brain and extra-brain activity) data for each camera.…”
Section: Methodsmentioning
confidence: 99%
“…This point was addressed by investigating the relevance of extra-brain activity which is not accounted for in a phantom study. The high uptake and retention of [ 123 I]FP-CIT in lungs, liver, and intestines and sometimes in salivary glands and thyroid [ 9 ] is, in fact, expected to contribute to the brain image, particularly through septal penetration from the 123 I high-energy gamma emissions [ 10 , 11 ]. The magnitude of this contribution was indirectly estimated from a comparison of the phantom (brain activity only) and the human (brain and extra-brain activity) data for each camera.…”
Section: Methodsmentioning
confidence: 99%
“…In both detectors, the DEW method is limited by the inability to account for spatial distribution of scattered photons (see above). Moreover, it relies on calibration of the k factor which is then applied indiscriminately to the acquired dataset, and DEW cannot account for downscatter from the 529 keV iodine-123 peak (28,29); both adaptations would require a third energy window above the photopeak window. In CZT detectors, overestimation of scatter using the DEW method will result from the detector-speci c low-energy tail which is caused by contamination from photons that are unscattered but detected with lower energy (28,30).…”
Section: Discussionmentioning
confidence: 99%
“…The corrected image was calculated as follows 25:where the subscript ds is used to indicate the downscatter window.…”
Section: Methodsmentioning
confidence: 99%