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Flight Performance of an advanced CZT Imaging Detector in a Balloon-borne Wide-Field Hard X-ray Telescope - ProtoEXIST1

机译:一架先进的CZT成像探测器的飞行性能   气球传播的宽视场硬X射线望远镜 - protoEXIsT1

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摘要

We successfully carried out the first high-altitude balloon flight of awide-field hard X-ray coded-aperture telescope ProtoEXIST1, which was launchedfrom the Columbia Scientific Balloon Facility at Ft. Sumner, New Mexico onOctober 9, 2009. ProtoEXIST1 is the first implementation of an advanced CdZnTe(CZT) imaging detector in our ongoing program to establish the technologyrequired for next generation wide-field hard X-ray telescopes. The CZT detectorplane in ProtoEXIST1 consists of an 8 x 8 array of closely tiled 2 cm x 2 cm x0.5 cm thick pixellated CZT crystals, each with 8 x 8 pixels, covering a 256cm^2 active area with 2.5 mm pixels. A tungsten mask, mounted at 90 cm abovethe detector provides shadowgrams of X-ray sources in the 30 - 600 keV band forimaging, allowing a fully coded field of view of 9 Deg x 9 Deg with an angularresolution of 20 arcmin. To reduce the background radiation, the detector issurrounded by semi-graded (Pb/Sn/Cu) passive shields on the four sides all theway to the mask. On the back side, a 26 cm x 26 cm x 2 cm CsI(Na) active shieldprovides signals to tag charged particle induced events as well as >~ 100 keVbackground photons from below. The flight duration was only about 7.5 hours dueto strong winds (60 knots) at float altitude (38-39 km). Throughout the flight,the CZT detector performed excellently. The telescope observed Cyg X-1 for ~ 1hour at the end of the flight. Despite a few problems with the pointing andaspect systems that caused the telescope to track about 6.4 deg off the target,the analysis of the Cyg X-1 data revealed an X-ray source at 7.2 sigma in the30-100 keV energy band at the expected location from the optical images takenby the onboard daytime star camera. The success of this first flight is veryencouraging for the future development of the advanced CZT imaging detectors(ProtoEXIST2, with 0.6 mm pixels).
机译:我们成功进行了全场硬X射线编码孔径望远镜ProtoEXIST1的高空气球飞行,该望远镜是从Ft的哥伦比亚科学气球设施发射的。新墨西哥州萨姆纳市,2009年10月9日。ProtoEXIST1是我们正在进行的计划中的先进CdZnTe(CZT)成像探测器的第一个实施方案,旨在建立下一代广角硬X射线望远镜所需的技术。 ProtoEXIST1中的CZT检测器平面由一个8 x 8阵列组成,这些阵列由紧密贴砖的2 cm x 2 cm x0.5 cm厚的像素化CZT晶体组成,每个晶体具有8 x 8像素,覆盖了256cm ^ 2的有效区域,具有2.5 mm像素。在检测器上方90厘米处安装的钨罩可提供30-600 keV波段的X射线源影影,以进行成像,从而实现9 Deg x 9 Deg的完全编码视场以及20 arcmin的角分辨率。为了减少背景辐射,检测器在通向掩模的四个侧面上均被半渐变(Pb / Sn / Cu)无源屏蔽层包围。在背面,一个26 cm x 26 cm x 2 cm CsI(Na)有源屏蔽提供信号来标记带电粒子引发的事件以及从下方发出的~~ 100 keV背景光子。由于在浮动高度(38-39公里)处有强风(60节),飞行时间仅为7.5小时左右。在整个飞行过程中,CZT探测器均表现出色。飞行结束后,望远镜观测了Cyg X-1约1小时。尽管定点和方面系统存在一些问题,导致望远镜跟踪距目标约6.4度,但对Cyg X-1数据的分析显示,在预期的30-100 keV能带中,存在一个7.2 sigma的X射线源。机载日间星型摄像机拍摄的光学图像中的位置。首次飞行的成功极大地鼓舞了先进CZT成像探测器(ProtoEXIST2,具有0.6毫米像素)的未来发展。

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