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Developments of scientific CMOS as focal plane detector for Einstein Probe mission

机译:科学CMOS作为用于爱因斯坦探测任务的焦平面探测器的发展

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China's Einstein Probe (EP) mission is designed for time-domain astrophysics with energy band of 0.5-4 keV. The payloads of EP include a wide-field X-ray telescope (WXT) and a follow-up X-ray telescope (FXT). The field of view (FOV) of WXT is about 3600 square degrees with sensitivity at least 10 times better than traditional X-ray all-sky monitors applying collimators or coded-masks. Back-side illuminated scientific CMOS (BSI sCMOS) is the best choice for WXT after several types of X-ray detectors are investigated. In this work, we study a BSI sCMOS sensor. GSENSE400BSI developed by Gpixel Inc.. which is treated as a pathfinder for the focal plane detector of WXT. GSENSE400BSI has a pixel array of 2048×2048 with pixel size of 11 μm. We have characterized this BSI sCMOS as an X-ray detector. Based on the excellent performance of GSENSE400BSI, a new BSI sCMOS device with large sensitive area of 6×6 cm~2 has been proposed as the focal plane detector for WXT.
机译:中国的爱因斯坦探测(EP)任务是为能带为0.5-4 keV的时域天体物理学设计的。 EP的有效载荷包括一个广角X射线望远镜(WXT)和一个后续X射线望远镜(FXT)。 WXT的视场(FOV)约为3600平方度,其灵敏度至少是使用准直仪或编码掩模的传统X射线全天候监视器的10倍。在研究了几种类型的X射线探测器之后,背面照明科学型CMOS(BSI sCMOS)是WXT的最佳选择。在这项工作中,我们研究了BSI sCMOS传感器。由Gpixel Inc.开发的GSENSE400BSI被视为WXT焦平面检测器的探路者。 GSENSE400BSI具有2048×2048的像素阵列,像素大小为11μm。我们已将此BSI sCMOS表征为X射线检测器。基于GSENSE400BSI的优异性能,提出了一种新型的BSI sCMOS器件,该器件具有6×6 cm〜2的大灵敏面积,可作为WXT的焦平面检测器。

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