Development of an optical photon-counting imager with a monolithic Geiger Avalanche Photodiode array

T. Nakamori, Yuga Ouchi, Risa Ogihara, T. Terasawa, Yuhei Kato, S. Shibata
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Abstract

We have developed a sensor system based on an optical photon-counting imager with high timing resolution, aiming for highly time-variable astronomical phenomena. The detector is a monolithic Geiger-mode avalanche photodiode array customized in a Multi-Pixel Photon Counter with a response time on the order of nanoseconds. This paper evaluates the basic performance of the sensor and confirms the gain linearity, uniformity, and low dark count. We demonstrate the system's ability to detect the period of a flashing LED, using a data acquisition system developed to obtain the light curve with a time bin of 100 microseconds. The Crab pulsar was observed using a 35-cm telescope without cooling, and the equipment detected optical pulses with a period consistent with the data from the radio ephemeris. Although improvements to the system will be necessary for more reliability, the system has been proven to be a promising device for exploring the time-domain optical astronomy.
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单片盖革雪崩光电二极管阵列光学光子计数成像仪的研制
针对高时变天文现象,我们开发了一种基于光学光子计数成像仪的高时序分辨率传感器系统。该探测器是一个单片盖革模式雪崩光电二极管阵列,在多像素光子计数器中定制,响应时间为纳秒级。本文对传感器的基本性能进行了评估,确定了传感器的增益线性度、均匀性和低暗计数。我们演示了该系统检测闪烁LED周期的能力,使用开发的数据采集系统来获得100微秒时间仓的光曲线。蟹状星云脉冲星是用一架35厘米的望远镜在没有冷却的情况下观测到的,该设备探测到的光脉冲周期与射电星历的数据一致。虽然为了提高系统的可靠性,还需要对系统进行改进,但该系统已被证明是探索时域光学天文学的一个有前途的设备。
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