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
{"title":"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","authors":"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","doi":"arxiv-2409.02356","DOIUrl":null,"url":null,"abstract":"We report on a free-space-coupled superconducting nanowire single-photon\ndetector array developed for NASA's Deep Space Optical Communications project\n(DSOC). The array serves as the downlink detector for DSOC's primary ground\nreceiver terminal located at Palomar Observatory's 200-inch Hale Telescope. The\n64-pixel WSi array comprises four quadrants of 16 co-wound pixels covering a\n320 micron diameter active area and embedded in an optical stack. The detector\nsystem also includes cryogenic optics for filtering and focusing the downlink\nsignal and electronics for biasing the array and amplifying the output pulses.\nThe detector system exhibits a peak system detection efficiency of 76% at 1550\nnm, a background-limited false count rate as low as 3.7 kcps across the array,\ntiming jitter less than 120 ps FWHM, and a maximum count rate of ~ 1 Gcps.","PeriodicalId":501374,"journal":{"name":"arXiv - PHYS - Instrumentation and Detectors","volume":"28 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"An SNSPD-based detector system for NASA's Deep Space Optical Communications project\",\"authors\":\"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\",\"doi\":\"arxiv-2409.02356\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We report on a free-space-coupled superconducting nanowire single-photon\\ndetector array developed for NASA's Deep Space Optical Communications project\\n(DSOC). The array serves as the downlink detector for DSOC's primary ground\\nreceiver terminal located at Palomar Observatory's 200-inch Hale Telescope. The\\n64-pixel WSi array comprises four quadrants of 16 co-wound pixels covering a\\n320 micron diameter active area and embedded in an optical stack. The detector\\nsystem also includes cryogenic optics for filtering and focusing the downlink\\nsignal and electronics for biasing the array and amplifying the output pulses.\\nThe detector system exhibits a peak system detection efficiency of 76% at 1550\\nnm, a background-limited false count rate as low as 3.7 kcps across the array,\\ntiming jitter less than 120 ps FWHM, and a maximum count rate of ~ 1 Gcps.\",\"PeriodicalId\":501374,\"journal\":{\"name\":\"arXiv - PHYS - Instrumentation and Detectors\",\"volume\":\"28 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-04\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Instrumentation and Detectors\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.02356\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Instrumentation and Detectors","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.02356","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
An SNSPD-based detector system for NASA's Deep Space Optical Communications project
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.