DSpace DSpace UPC
 Català   Castellano   English  

E-prints UPC >
Altres >
Enviament des de DRAC >

Empreu aquest identificador per citar o enllaçar aquest ítem: http://hdl.handle.net/2117/11171

Ítem no disponible en accés obert per política de l'editorial

Arxiu Descripció MidaFormat
01466779.pdf970,73 kBAdobe PDF Accés restringit

Citació: Cot, A. [et al.]. Modelling of high-energy contamination in SPECT imaging using Monte Carlo simulation. A: Nuclear Science Symposium and Medical Imaging Conference. "IEEE Nuclear Science Symposium and Medical Imaging Conference 2004". Roma: IEEE, 2004, p. 4028-4031.
Títol: Modelling of high-energy contamination in SPECT imaging using Monte Carlo simulation
Autor: Cot Sanz, Alberto Veure Producció científica UPC; Jané, E; Sempau Roma, Josep Veure Producció científica UPC; Falcón, C; Bullich, S; Pavía, J; Calviño Tavares, Francisco Veure Producció científica UPC; Ros, D
Editorial: IEEE
Data: 2004
Tipus de document: Conference report
Resum: 3I is a commonly used radioisotope employed in neurotransmitter SPECT studies. In addition to an intense line at 159 keV, the decay scheme of this radioisotope includes a low yield (∼3%) of higher energy photons which have a non-negligible contribution to the final image when low-energy high-resolution (LEHR) collimators are used. This contribution of high-energy photons may achieve ∼28% of the total counts in the projections. The aim of this work is to model each energy component of the high-energy Point Spread Function (hPSF) for fan-beam LEHR collimators in order to develop faster Monte Carlo (MC) simulations of high-energy ray contamination. The modelling of hPSF was based on the results of simulating photons through the collimator-detector system using the MC code PENELOPE. Since low-energy PSFs models for fan-beam collimators must tend to a Gaussian distribution, we use the same function for the hPSF modelling for high-energy photons. The parameters of these Gaussian functions were obtained by minimizing the root mean square (RMS) error between each simulated hPSF and the function g(x, y) using the efficiency of the simulated hPSFs as a constraint. The RMS attained with fit of g(x, y) to the simulated hPSFs was always smaller than ∼2% of the mean efficiency per pixel of the image. A very strong dependence of the efficiency on the type and thickness of the backscatter material behind the crystal was found. The hPSFs were parameterized for a wide range of energies, ranging from 350 keV to 538 keV. Our results indicate that Gaussian distributions approximate in a suitable way the hPSF responses for fan-beam collimators. This model will be an important tool to accelerate MC simulations of radiolabelled compounds which emit medium- or high-energy rays.
URI: http://hdl.handle.net/2117/11171
Versió de l'editor: URL: http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=1466779&isnumber=31439
Apareix a les col·leccions:GREENER - Grup de recerca d´estudis energètics i de les radiacions. Ponències/Comunicacions de congressos
Departament de Física i Enginyeria Nuclear. Ponències/Comunicacions de congressos
Altres. Enviament des de DRAC
Institut de Tècniques Energètiques. Ponències/Comunicacions de congressos

Stats Mostra les estadístiques d'aquest ítem

SFX Query

Aquest ítem (excepte textos i imatges no creats per l'autor) està subjecte a una llicència de Creative Commons Llicència Creative Commons
Creative Commons


Valid XHTML 1.0! Programari DSpace Copyright © 2002-2004 MIT and Hewlett-Packard Comentaris
Universitat Politècnica de Catalunya. Servei de Biblioteques, Publicacions i Arxius