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Symbia t16 spect ct system

Manufactured by Siemens

The Symbia T16 SPECT/CT system is a medical imaging device designed for Single Photon Emission Computed Tomography (SPECT) and Computed Tomography (CT) imaging. It combines the functional information from SPECT with the anatomical detail of CT to provide comprehensive diagnostic information.

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2 protocols using symbia t16 spect ct system

1

Multimodal Imaging Protocol for Bone SPECT and CT

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We used 11 clinical SPECT and 12 clinical CT images in this study. The SPECT scans were acquired on a Siemens Symbia T16 SPECT/CT system. The bone SPECT acquisitions were performed using our clinical bone SPECT protocol (120 views per bed position, and two energy windows with widths of 15% and centered at 140 KeV and 119 keV with the latter serving as a scatter window), followed by CT acquisition. The clinical CT images were acquired from 12 patients, with 8 on the Siemens SPECT/CT system and 4 on a GE CT system. Both SPECT and CT images were reconstructed using scanner software. The SPECT reconstructions were obtained using Flash 3D/OS-EM (with default numbers of iteration and subsets) with attenuation, energy-window-based scatter, and geometric collimator-detector response compensations enabled. Bone and lesion in the SPECT and CT images were manually delineated by consensus of two experienced radiologists, where the initial segmentation was produced by a radiology fellow and verified by an attending physician. Two different fellows produced the initial segmentations.
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2

SPECT/CT Imaging Protocol Optimization

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Conventional SPECT/CT imaging was performed with a dual-head Siemens Symbia T16 SPECT/CT system, equipped with medium-energy general-purpose parallel-hole collimators. Acquisition parameters of the CT scan were set to 130 kV, 30 mAs, and 0.97×0.97×5mm3 voxel size while the SPECT scanning protocol followed the protocol described by Marin et al. [8 (link)] with the following parameters: a 128×128 matrix, voxel size of 4.79 mm, 32 views with 30 s per view, and an energy window centered at the 208 keV photopeak (with a 20% width) combined with a lower scatter window (with a 10% width). The projection data were decay and scatter corrected and reconstructed using Ordered Subsets Expectation Maximization (OSEM) [9 (link)]. To optimize the reconstruction protocol such that sphere-to-background ratios were as close as possible to the true ratio while keeping the noise level as low as possible, the number of iterations and subsets were gradually increased (4i4s, 8i8s, 16i16s and 24i16s) with 16 the highest possible number of subsets. In addition, default post-smoothing was performed with a Gaussian filter of 1 mm Full width half maximum (FWHM), with additional filtering being considered to further reduce the noise if necessary.
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