首页> 外文会议>INTEGRAL Workshop on The INTEGRAL Universe >IMAGE RECONSTRUCTION FOR THE MEGA TELESCOPE
【24h】

IMAGE RECONSTRUCTION FOR THE MEGA TELESCOPE

机译:Mega望远镜的图像重建

获取原文

摘要

The Compton scattering and pair creation telescope MEGA detects gamma-rays in the energy range from 400 keV up to at least 50 MeV. Its multidimensional response presents a challenge for image reconstruction: The large amount of measured parameters and the geometry result in a response, which depends on incidence angle, energy, Compton scatter angle, direction and energy of scattered electrons, etc. Moreover the image reconstruction algorithm has to incorporate different event types into one image (tracked und untracked Compton events as well as pair events) and has to cope with high background conditions. An algorithm, which meets this challenges, is the iterative List-Mode Maximum-Likelihood Expectation-Maximization algorithm. The adoptions of this algorithm to the needs of the MEGA telescope are shown along with selected results.
机译:康普顿散射和配对创建望远镜巨型率检测到400 kev的能量范围内的伽马射线,高达50米。其多维响应对图像重建提出了挑战:大量测量参数和几何形状的响应导致响应,这取决于散射电子的入射角,能量,康普顿散射角,方向和能量等。此外,散射电子等的响应等。此外,散射电子的方向和能量等等必须将不同的事件类型纳入一个图像(跟踪Untacked Compton事件以及对事件),并且必须应对高背景条件。一种符合这项挑战的算法是迭代列表模式最大似然预期最大化算法。将该算法的采用与选定的结果一起显示了Mega望远镜的需要。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号