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New concept large area, narrow field CZT telescope for formation flying

机译:新概念大面积,窄场CZT望远镜用于编队飞行

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The development of formation flying technology in space has opened a new window for astronomy at hard X-γ-ray wavelenghts, allowing observations with unprecedented angular resolution (location accuracy of the order of few arcsec). This has stimulated the development of new concepts for imaging instruments: on one side, the focusing telescopes like γ-ray lens, using small,well shielded detector volumes, on the other side very large area γ-ray imagers, both allowing a big step in sensitivity. We report on a study for the concept of a large area (1 square meter), narrow field coded mask telescope with arcsec imaging capability, based on CZT detector technology and active collimation system, made of Si microstrip detector modules and operating in the energy band 15-500 keV. Feasibility and performance characteristics are discussed as well as possible geometric configurations and background suppression schemes, in the light of data obtained from INTEGRAL/IBIS and other CdTe/CZT instruments currently in space.
机译:太空编队飞行技术的发展为硬X-γ射线波长的天文学开辟了新的窗口,允许以前所未有的角分辨率(几弧秒量级的定位精度)进行观测。这激发了成像仪器新概念的发展:一方面,聚焦望远镜(如γ射线透镜)使用体积小且屏蔽良好的检测器;另一方面,非常大面积的γ射线成像仪,都允许较大的步进在敏感性上。我们报告了一项基于CZT探测器技术和有源准直系统,由Si微带探测器模块制成并在能带中工作的大面积(1平方米),具有arcsec成像功能的窄场编码掩模望远镜的概念的研究15-500 keV。根据从INTEGRAL / IBIS和当前空间中其他CdTe / CZT仪器获得的数据,讨论了可行性和性能特征以及可能的几何配置和背景抑制方案。

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