首页> 外文会议>Conference on X-Ray and Gamma-Ray Instrumentation for Astronomy XI 2-4 August 2000 San Diego, USA >Construction and Testing of a Pixellated CZT Detector and Shield for a Hard X-ray Astronomy Balloon Flgiht
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Construction and Testing of a Pixellated CZT Detector and Shield for a Hard X-ray Astronomy Balloon Flgiht

机译:硬X射线天文学气球飞行的像素化CZT检测器和防护罩的构造和测试

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We report on the construction and laboratory testing of pixellated CZT detectors mounted in a flip-chip, tiled fashion and read out by an ASIC, as required for proposed hard X-ray astronomy missions. Two 10 mm x 10 mm x 5 mm detectors were fabricated, oen out of standard eV Products high-presusre Bridgman CZT and one out of IMARAD horizontal Bridgman CZT. Each was fashioned with a 4 x 4 array of gold pixels on a 2.5 mm pitchw ith a surrounding guard ring. The detectors were mounted sid by side on a carrier card, such that the pixel pitch was preserved, and read out by a 32-channel VA-TA ASIC from IDE AS Corp. controlled by a PC/104-single-board computer. A passive shield/collimator surrounded by plastic scintillator encloses the detectors on five sides and provides a approx 40 deg field of view. Thus this experiment tests key techniques required for future hard X-ray survey instruments. The experiment was taken to Ft Sumner, NM in May 2000 in preparation for a scientific balloon flight aboard the joint Harvard-MSFC EXITE2/HERO payload. Although we did not receive a flight opportunity, and are currently shceduled to fly in September 2000, we present our calibration data in the flight configuration together with data anlysis techniques and simulations fo the expected flight background spectrum.
机译:我们报告了以倒装芯片,平铺方式安装并由ASIC读出的像素化CZT探测器的构造和实验室测试,这是拟议的硬X射线天文学任务所需的。装配了两个10毫米x 10毫米x 5毫米探测器,它们是从标准eV产品高清晰度Bridgman CZT中选出的,而一个是从IMARAD水平Bridgman CZT中选出的。每个镜框均由2.5毫米间距的4 x 4金色像素阵列和周围的保护环构成。将检测器并排安装在载体卡上,以保持像素间距,并由PC / 104单板计算机控制的IDE AS Corp.的32通道VA-TA ASIC读出。被塑料闪烁体包围的无源屏蔽/准直仪在五个侧面将探测器围住,并提供约40度的视野。因此,该实验测试了未来硬X射线测量仪器所需的关键技术。该实验于2000年5月在新罕布什尔州萨姆纳堡进行,以准备在联合的哈佛-MSFC EXITE2 / HERO载荷上进行科学气球飞行。尽管我们没有获得任何飞行机会,并且目前已于2000年9月开始飞行,但我们还是将飞行数据中的校准数据与数据分析技术和模拟一起提供了预期的飞行背景光谱。

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