TABLE 1

Parameters Commonly Used for SPECT Recording and Reconstruction

ParameterDiscovery NM 530cDSPECTIQ⋅SPECTConventional SPECT
Recording
 CollimatorMultipinholeWide-angle parallel holeAstigmaticLEHR or parallel hole
 Energy window140 keV ± 10%140 keV ± 10%140 keV ± 7.5%140 keV ± 7.5%
 Number of projections19120 (×9 blocks)17 (×2 heads)16 (×2 heads)
 Detector angle between consecutive projectionsNone (fixed detector)0.4°–7°*
Reconstruction
 MethodIterative 3DIterative 3DIterative 3DIterative 3D
 Number of iterations607108
 Number of subsets13234
 Interiteration filterKernel (0.125)
 Final filterButterworth (order, 7; cutoff, 0.37 cm−1)Normalizing filterGaussian (10 mm FWHM)Gaussian (10 mm FWHM)
 Pixel size (mm)4.04.924.86.6
  • * Angles are approximately 0.4° for projections passing through cardiac region (as defined by adjusted region of interest on prescan images) and up to 7° for other projections.

  • Way in which normalizing filter works is proprietary information of Spectrum Dynamics.

  • LEHR = low-energy high-resolution; 3D = 3-dimensional; FWHM = full width at half maximum.