Performance of a Compton telescope using position-sensitive germanium detectors

B. Phlips, S. Inderhees, R. Kroeger, W. Johnson, R. Kinzer, J. Kurfess, B. Graham, N. Gehrels
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引用次数: 13

Abstract

We describe the use of position sensitive planar germanium detectors in a Compton telescope/camera. This Compton telescope achieves the very good energy resolution (/spl Delta/Etotal<4 keV) associated with germanium detectors and good position resolution (2 mm). By combining a 25/spl times/25 strip (2 mm pitch) detector with a 5/spl times/5 strip detector (9 mm pitch), we created a telescope with 625/spl times/25 pixel combinations. Using this detector pair, we have reconstructed positions with an angular resolution of 1 degree FWHM and 15 arcminute centroiding. Point sources are identified with less than 100 full energy events with simple image reconstruction. The angular resolution is currently limited by the uncertainty in the absolute position of the detectors and the size of the second detector pixels. We show the expected angular resolution when the pixel size no longer dominates the angular resolution and discuss proposed applications.
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使用位置敏感锗探测器的康普顿望远镜的性能
我们描述了位置敏感平面锗探测器在康普顿望远镜/照相机中的应用。这台康普顿望远镜实现了与锗探测器相关的非常好的能量分辨率(/spl Delta/Etotal<4 keV)和良好的位置分辨率(2 mm)。通过将25/spl倍/25条(2 mm间距)探测器与5/spl倍/5条探测器(9 mm间距)相结合,我们创造了一个625/spl倍/25像素组合的望远镜。利用这对探测器,我们重建了角度分辨率为1度FWHM和15弧分质心的位置。通过简单的图像重建,以小于100个全能量事件识别点源。角度分辨率目前受到探测器绝对位置的不确定性和第二探测器像素大小的限制。我们展示了当像素大小不再支配角分辨率时的预期角分辨率,并讨论了拟议的应用。
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