An SNSPD-based detector system for NASA's Deep Space Optical Communications project

Emma E. Wollman, Jason P. Allmaras, Andrew D. Beyer, Boris Korzh, Marcus C. Runyan, Lautaro Narváez, William H. Farr, Francesco Marsili, Ryan M. Briggs, Gregory J. Miles, Matthew D. Shaw
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Abstract

We report on a free-space-coupled superconducting nanowire single-photon detector array developed for NASA's Deep Space Optical Communications project (DSOC). The array serves as the downlink detector for DSOC's primary ground receiver terminal located at Palomar Observatory's 200-inch Hale Telescope. The 64-pixel WSi array comprises four quadrants of 16 co-wound pixels covering a 320 micron diameter active area and embedded in an optical stack. The detector system also includes cryogenic optics for filtering and focusing the downlink signal and electronics for biasing the array and amplifying the output pulses. The detector system exhibits a peak system detection efficiency of 76% at 1550 nm, a background-limited false count rate as low as 3.7 kcps across the array, timing jitter less than 120 ps FWHM, and a maximum count rate of ~ 1 Gcps.
美国国家航空航天局深空光通信项目基于 SNSPD 的探测器系统
我们报告了为美国国家航空航天局深空光通信项目(DSOC)开发的自由空间耦合超导纳米线单光电探测器阵列。该阵列是 DSOC 位于帕洛玛天文台 200 英寸黑尔望远镜的主要地面接收终端的下行链路探测器。WSi 64 像素阵列由四个象限的 16 个共同缠绕像素组成,覆盖直径为320 微米的有效区域,并嵌入一个光学堆栈中。探测器系统还包括用于过滤和聚焦下行链路信号的低温光学系统,以及用于偏置阵列和放大输出脉冲的电子设备。该探测器系统在 1550nm 波长下的峰值系统探测效率为 76%,整个阵列的背景限制误计数率低至 3.7 kcps,定时抖动小于 120 ps FWHM,最大计数率约为 1 Gcps。
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