Hunter William C J, Barrett Harrison H, Furenlid Lars R
Department of Radiology, University of Washington, Seattle, WA 98195 USA (
IEEE Trans Nucl Sci. 2009 Feb 10;56(1):189-196. doi: 10.1109/TNS.2008.2010704.
High-energy (> 100 keV) photon detectors are often made thick relative to their lateral resolution in order to improve their photon-detection efficiency. To avoid issues of parallax and increased signal variance that result from random interaction depth, we must determine the 3D interaction position in the imaging detector. With this goal in mind, we examine a method of calibrating response statistics of a thick-detector gamma camera to produce a maximum-likelihood estimate of 3D interaction position. We parameterize the mean detector response as a function of 3D position, and we estimate these parameters by maximizing their likelihood given prior knowledge of the pathlength distribution and a complete list of camera signals for an ensemble of gamma-ray interactions. Furthermore, we describe an iterative method for removing multiple-interaction events from our calibration data and for refining our calibration of the mean detector response to single interactions. We demonstrate this calibration method with simulated gamma-camera data. We then show that the resulting calibration is accurate and can be used to produce unbiased estimates of 3D interaction position.
高能(> 100 keV)光子探测器相对于其横向分辨率通常做得较厚,以提高其光子探测效率。为避免因随机相互作用深度而导致的视差问题和信号方差增加,我们必须确定成像探测器中的三维相互作用位置。出于这一目的,我们研究了一种校准厚探测器伽马相机响应统计数据的方法,以生成三维相互作用位置的最大似然估计。我们将探测器平均响应参数化为三维位置的函数,并通过在已知路径长度分布和一组伽马射线相互作用的相机信号完整列表的先验知识的情况下最大化其似然性来估计这些参数。此外,我们描述了一种迭代方法,用于从校准数据中去除多次相互作用事件,并完善我们对探测器对单次相互作用的平均响应的校准。我们用模拟伽马相机数据演示了这种校准方法。然后我们表明,所得校准是准确的,可用于生成三维相互作用位置的无偏估计。