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A 9 megapixel large-area back-thinned CMOS sensor with high sensitivity and high frame-rate for the TAOS Ⅱ program

机译:适用于TAOSⅡ程序的9兆像素大面积背照式CMOS传感器,具有高灵敏度和高帧率

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The Transneptunian Automated Occultation Survey (TAOS Ⅱ) is a robotic telescope system using three telescopes in San Pedro Martir Observatory in Mexico. It measures occultation of background stars by small TransNeptunian Objects (TNO) in order to determine their size distribution. Each telescope focal plane uses ten buttable backthinned CMOS sensors. Key performance features of the sensors are: Large array format 4608 × 1920, Pixel size 16μm, Multi ROIs, 8 analogue video channels, Frame rate of 20-40 fps [using ROIs], Low noise <3e-, Cryogenic dark current <0.1e~-/pixel/s, backthinned for >90% peak quantum efficiency. The paper describes top level application requirements for the TAOS Ⅱ detector. The sensor design including the pixel and buttable package are described together with performance at room temperature and cryogenic temperature of backthinned devices. The key performance specifications have been demonstrated and will be presented. The production set of 40 devices are due for completion within 2017.
机译:Transneptunian自动掩星调查(TAOSⅡ)是在墨西哥的San Pedro Martir天文台使用三个望远镜的机器人望远镜系统。它可以测量小型跨海王星天体(TNO)对背景恒星的遮蔽,以确定其大小分布。每个望远镜焦平面都使用十个可调节的背面变薄CMOS传感器。传感器的主要性能特点是:大阵列格式4608×1920,像素大小16μm,多ROI,8个模拟视频通道,帧速率20-40 fps(使用ROI),低噪声<3e-,低温暗电流<0.1 e〜-/ pixel / s,后缩小以达到大于90%的峰值量子效率。本文介绍了TAOSⅡ检测器的最高应用要求。描述了包括像素和对接封装在内的传感器设计,以及背面变薄器件在室温和低温下的性能。关键性能规格已得到演示,并将介绍。 40套设备的生产套件将于2017年内完成。

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