The current projects of future X-rays space telescopes foresee high resolving power transition edge sensor (TES) micro-calorimeters arrays as focal plane instrument. In order to full exploit their sensitivity in the space environment, they need an anticoincidence detector to reject the background due to cosmic charged particles. High-energy protons (> 150 MeV) and other charged particle may release in the X-ray calorimeter, the same energy of the X-rays sources under observation. We report the description of the last prototype based on TES calorimeter where a 1-cm 2 silicon chip is used as both substrate and absorber. The readout is made of 96 iridium/gold TESs uniformly distributed on its surface and parallel wired. In this paper, we will describe the design, with the preliminary phonon dynamics simulation, the fabrication, of first demonstration model for the ATHENA space telescope project.

中文翻译：

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雅典娜X射线望远镜焦平面声子介导TES宇宙射线探测器

未来 X 射线空间望远镜的当前项目预见高分辨率转换边缘传感器 (TES) 微量热仪阵列作为焦平面仪器。为了充分利用它们在空间环境中的敏感性，它们需要一个反重合探测器来拒绝宇宙带电粒子造成的背景。高能质子 (> 150 MeV) 和其他带电粒子可能会在 X 射线量热仪中释放，与所观察的 X 射线源的能量相同。我们报告了基于 TES 热量计的最后一个原型的描述，其中 1 厘米 2 硅芯片用作基板和吸收器。读数由 96 个均匀分布在其表面并平行布线的铱/金 TES 制成。在本文中，我们将通过初步声子动力学模拟、制造、