首页> 外文会议>Conference on High-Energy Detectors in Astronomy; 20040622-20040623; Glasgow; GB >Performance of a Gas Scintillation Proportional Counter Array for a High-Energy X-Ray Observatory
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Performance of a Gas Scintillation Proportional Counter Array for a High-Energy X-Ray Observatory

机译:高能X射线天文台气体闪烁比例计数器阵列的性能

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A focal plane array of high-pressure gas scintillation proportional counters (GSPC) for a High Energy X-Ray Observatory (HERO) has been developed at the Marshall Space Flight Center. The array consists of eight GSPCs and is a part of balloon-born payload scheduled to fly in May 2004. These detectors have an active area of ~ 20 cm~2 each, and are filled with a high pressure (10~6 Pa) xenon-helium mixture. Imaging is via crossed-grid position-sensitive phototubes sensitive in the UV region. The performance of the GSPC is well matched to that of the telescope's x-ray optics which have response to 75 keV and a focal spot size of ~ 0.5 mm. The detector's energy resolution, 5.0% FWHM at 60 keV, is adequate for resolving the broad spectral lines of astrophysical importance and for accurate continuum measurements. Results of the ground detector array testing are presented.
机译:在马歇尔太空飞行中心开发了用于高能X射线天文台(HERO)的高压气体闪烁比例计数器(GSPC)的焦平面阵列。该阵列由八个GSPC组成,是计划于2004年5月飞行的气球载有效载荷的一部分。这些探测器的有效面积各为〜20 cm〜2,并充满高压(10〜6 Pa)氙气-氦混合物。通过在紫外线区域敏感的交叉栅格位置敏感光电管进行成像。 GSPC的性能与望远镜的X射线光学器件非常匹配,后者可响应75 keV,焦点尺寸约为0.5 mm。该探测器的能量分辨率为60 keV,FWHM为5.0%FWHM,足以解决具有天体物理学重要性的宽光谱线并进行准确的连续测量。给出了地面探测器阵列测试的结果。

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