imgfiltg 0.4.0 © 2006-2013 by Turku PET Centre

Program for applying 2D or 3D Gaussian filter for a static or dynamic PET image (ECAT 6.3, 7.x or Analyze 7.5 format). SD of Gaussian filter must be specified by user, and SD=FWHM/2.355. 2D convolution is slow in case of large image and large filter size, but more accurate than fast 2D and 3D algorithms. Command line arguments: 1) dynamic PET image file 2) Gaussian filtered image file 3) SD of Gaussian filter (by default in pixels; see below) Options: -method=<<2D>|<fast2D>|<fast3D>> Specify the Gaussian filtering method; default is the 2D convolution method which is slow but accurate; fast2D is a less accurate but fast 2D Gaussian convolution algorithm with IIR approximation; fast3d is 3D Gaussian convolution algorithm with IIR approximation. -border=<fill|zero> Image is extrapolated symmetrically before smoothing (fill, default), or data outside image borders is assumed to be zeroes (zero). Applies only to 2D method. -fsize=<filter size>[pxl|mm|cm] Size of filter kernel, by default 6*SD; size can be be given in pixels (default), mm, or cm. Final size in pixels will be automatically changed to the next odd number. Applies only to 2D method. -steps=<nr> More steps provides better accuracy but longer execution time; default is 4. Applies only to fast2D and fast3D methods. -pixelsize=<value> Set image pixel size (mm), if missing or wrong in image data. -h or --help Print this message and exit. --version or --build Print software build information and exit. --silent Program works silently, printing only error and warning messages. --verbose Program prints more information about what it is doing. Example #1a: Gaussian SD in pixels imgfiltg s5998dy1.v s5998dy1_filt.v 6pxl Example #1b: Gaussian with SD of 6 millimeters and 40 mm filter size imgfiltg -fsize=40mm s5998dy1.v s5998dy1_filt.v 6mm See also: imgdysmo, eflexseg, ecatthrs, ebkgrm, fvar4img, prfpeak, fitprfs Keywords: image, gaussian, filter, FWHM This program comes with ABSOLUTELY NO WARRANTY. This is free software, and you are welcome to redistribute it under GNU General Public License.

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Last updated 2013-03-08 11:38:30