2006
DOI: 10.1117/12.653300
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A new approach of 3D SPECT reconstruction for near-field coded aperture imaging

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Cited by 7 publications
(10 citation statements)
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“…While our previous results were quite encouraging, the objects we imaged were comprised of rods or capillary tubes that were with strong contrast and sharp edges [1][2][3]. It would be of interest to see how the proposed methods perform on objects with low contrast and slow variations that are common in small animal and medical imaging.…”
Section: Introduction S Ingle Photon Emission Computerized Tomogramentioning
confidence: 89%
“…While our previous results were quite encouraging, the objects we imaged were comprised of rods or capillary tubes that were with strong contrast and sharp edges [1][2][3]. It would be of interest to see how the proposed methods perform on objects with low contrast and slow variations that are common in small animal and medical imaging.…”
Section: Introduction S Ingle Photon Emission Computerized Tomogramentioning
confidence: 89%
“…In this article, we extend our previous research 14,22 and present a novel 3D image reconstruction approach to SPECT based on near-field coded aperture collimation and maximum likelihood estimation. The article is organized as follows.…”
Section: Introductionmentioning
confidence: 96%
“…To account for this depth dependent magnification, we developed a modified MLEM method to reconstruct a 3D image stack from a single coded aperture projection. In this method, the image slice at depth z is updated by 14,22 …”
Section: Iia1 Partial Reconstruction Of 3d Image Stack From Singlementioning
confidence: 99%
“…Among conventional methods, high-resolution collimations (e.g., pinhole) often yield low sensitivity, while high-sensitivity collimations (e.g., parallel-hole) generate images with poor resolution. To accommodate both, coded aperture (CA) collimation has been proposed as a potential method to achieve reasonably high sensitivity and high resolution in SPECT imaging [ 9 – 14 ]. This collimation technique was originally devised for astronomical imaging, where incoming projections from a given source (such as a star) are parallel [ 15 17 ].…”
Section: Introductionmentioning
confidence: 99%
“…In previous studies [ 9 , 11 , 12 ], it was discovered that the angular artifacts due to the aperture collimation effect of CA imaging is mostly neglected by researchers in the field. A solution has been proposed to correct for this collimation effect [ 12 ].…”
Section: Introductionmentioning
confidence: 99%