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A three-dimensional CZT detector as a focal plane prototype for a Laue Lens telescope

机译:三维CZT探测器作为劳厄透镜望远镜的焦平面原型

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The importance of hard X-ray astronomy (>10 keV) is now widely recognized. Recently both ESA and NASA have indicated in their guidelines for the progress of X- and γ-ray astronomy in the next decade the development of new instrumentation working in the energy range from the keV to the MeV region, where important scientific issues are still open, exploiting high sensitivity for spectroscopic imaging and polarimetry observations. The development of new concentrating (e.g. multilayer mirror) telescopes for hard X-rays (10-100 keV) and focusing instruments based on Laue lenses operating from ~60 keV up to a few MeV is particularly challenging. We describe the design of a three-dimensional (3D) depth-sensing position sensitive device suitable for use as the basic unit of a high efficiency focal plane detector for a Laue lens telescope. The sensitive unit is a drift strip detector based on a CZT crystal, (10 ×10 mm~2 area, 2.5 mm thick), irradiated transversally to the electric field direction. The anode is segmented into 4 detection cells, each comprising one collecting strip and 8 drift strips. The drift strips are biased by a voltage divider, whereas the anode strips are held at 0 V. The cathode is divided in 4 horizontal strips for the reconstruction of the Z interaction position. The 3D prototype will be made by packing 8 linear modules, each composed of 2 basic sensitive units, bonded onto a ceramic layer together with the readout electronics.
机译:硬X射线天文学(> 10 keV)的重要性现在广泛认可。最近,ESA和NASA都在下一年在X-γ射线天文学进展的指导方针中表明,从凯夫到MEV地区的能源范围内的新仪器的开发,重要的科学问题仍然开放,利用高灵敏度的光谱成像和偏振偏振物观察。新浓缩(例如多层镜子)用于硬X射线(10-100keV)和基于Laue镜头的聚焦仪器的开发,从〜60 kev的Laue镜片到几个MEV,尤其具有挑战性。我们描述了适用于用于Laue镜头望远镜的高效率焦平面检测器的基本单元的三维(3D)深度感测位置敏感装置的设计。敏感单元是基于CZT晶体的漂移条检测器(10×10mm〜2面积,2.5mm厚),横向地照射到电场方向。阳极被分段为4个检测单元,每个检测电池包括一个收集条和8个漂移条。漂移条由分压器偏置,而阳极带保持在0V。阴极被分成4个水平条带,用于重建Z相互作用位置。 3D原型将通过填充8个线性模块,每个模块由2个基本敏感单元组成,与读出电子器件一起粘合到陶瓷层上。

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