M. Salatino, J. Austermann, K. Thompson, P. Ade, Xiran Bai, J. Beall, D. Becker, Yi-Fu Cai, Z. Chang, Din Chen, Pisin Chen, J. Connors, J. Delabrouille, B. Dober, S. Duff, G. Gao, Shamik Ghosh, Richard C. Givhan, G. Hilton, B. Hu, J. Hubmayr, E. Karpel, C. Kuo, Hong Li, Mingzhe Li, Siyu Li, Xufang Li, Yongping Li, M. Link, Hao Liu, Liyong Liu, Yang Liu, F. Lu, Xue-Feng Lu, Tammy Lukas, J. Mates, Justin Mathewson, P. Mauskopf, J. Meinke, Jordi A. Montana-Lopez, Jenna Moore, Jingyan Shi, A. Sinclair, Ryan Stephenson, Wei Sun, Y. Tseng, C. Tucker, J. Ullom, L. Vale, J. Lanen, M. Vissers, S. Walker, Bo Wang, Guofeng Wang, Jiaxin Wang, E. Weeks, Di Wu, Yi-han Wu, J. Xia, Hexuan Xu, Ji Yao, Yong-qiang Yao, K. Yoon, B. Yue, Hua-jin Zhai, Aimei Zhang, Laiyu Zhang, Le Zhang, Pengjie Zhang, Tong Zhang, Xinmin Zhang, Yifei Zhang, Yongjie Zhang, Gong-Bo Zhao, Wen Zhao
{"title":"阿里微波背景偏振望远镜接收机的设计","authors":"M. Salatino, J. Austermann, K. Thompson, P. Ade, Xiran Bai, J. Beall, D. Becker, Yi-Fu Cai, Z. Chang, Din Chen, Pisin Chen, J. Connors, J. Delabrouille, B. Dober, S. Duff, G. Gao, Shamik Ghosh, Richard C. Givhan, G. Hilton, B. Hu, J. Hubmayr, E. Karpel, C. Kuo, Hong Li, Mingzhe Li, Siyu Li, Xufang Li, Yongping Li, M. Link, Hao Liu, Liyong Liu, Yang Liu, F. Lu, Xue-Feng Lu, Tammy Lukas, J. Mates, Justin Mathewson, P. Mauskopf, J. Meinke, Jordi A. Montana-Lopez, Jenna Moore, Jingyan Shi, A. Sinclair, Ryan Stephenson, Wei Sun, Y. Tseng, C. Tucker, J. Ullom, L. Vale, J. Lanen, M. Vissers, S. Walker, Bo Wang, Guofeng Wang, Jiaxin Wang, E. Weeks, Di Wu, Yi-han Wu, J. Xia, Hexuan Xu, Ji Yao, Yong-qiang Yao, K. Yoon, B. Yue, Hua-jin Zhai, Aimei Zhang, Laiyu Zhang, Le Zhang, Pengjie Zhang, Tong Zhang, Xinmin Zhang, Yifei Zhang, Yongjie Zhang, Gong-Bo Zhao, Wen Zhao","doi":"10.1117/12.2560709","DOIUrl":null,"url":null,"abstract":"AliCPT-1 is the first CMB degree scale polarimeter to be deployed to the Tibetan plateau at 5,250m asl. AliCPT-1 is a 95/150GHz 72cm aperture, two lens refracting telescope cooled down to 4K. Alumina lenses image the CMB on a 636mm wide focal plane. The modularized focal plane consists of dichroic polarization-sensitive Transition-Edge Sensors (TESes). Each module includes 1,704 optically active TESes fabricated on a 6in Silicon wafer. Each TES array is read out with a microwave multiplexing with a multiplexing factor up to 2,000. Such large factor has allowed to consider 10's of thousands of detectors in a practical way, enabling to design a receiver that can operate up to 19 TES arrays for a total of 32,300 TESes. AliCPT-1 leverages the technological advancements of AdvACT and BICEP-3. The cryostat receiver is currently under integration and testing. Here we present the AliCPT-1 receiver, underlying how the optimized design meets the experimental requirements.","PeriodicalId":393026,"journal":{"name":"Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X","volume":"339 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-12-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"18","resultStr":"{\"title\":\"The design of the Ali CMB Polarization Telescope receiver\",\"authors\":\"M. Salatino, J. Austermann, K. Thompson, P. Ade, Xiran Bai, J. Beall, D. Becker, Yi-Fu Cai, Z. Chang, Din Chen, Pisin Chen, J. Connors, J. Delabrouille, B. Dober, S. Duff, G. Gao, Shamik Ghosh, Richard C. Givhan, G. Hilton, B. Hu, J. Hubmayr, E. Karpel, C. Kuo, Hong Li, Mingzhe Li, Siyu Li, Xufang Li, Yongping Li, M. Link, Hao Liu, Liyong Liu, Yang Liu, F. Lu, Xue-Feng Lu, Tammy Lukas, J. Mates, Justin Mathewson, P. Mauskopf, J. Meinke, Jordi A. Montana-Lopez, Jenna Moore, Jingyan Shi, A. Sinclair, Ryan Stephenson, Wei Sun, Y. Tseng, C. Tucker, J. Ullom, L. Vale, J. Lanen, M. Vissers, S. Walker, Bo Wang, Guofeng Wang, Jiaxin Wang, E. Weeks, Di Wu, Yi-han Wu, J. Xia, Hexuan Xu, Ji Yao, Yong-qiang Yao, K. Yoon, B. Yue, Hua-jin Zhai, Aimei Zhang, Laiyu Zhang, Le Zhang, Pengjie Zhang, Tong Zhang, Xinmin Zhang, Yifei Zhang, Yongjie Zhang, Gong-Bo Zhao, Wen Zhao\",\"doi\":\"10.1117/12.2560709\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"AliCPT-1 is the first CMB degree scale polarimeter to be deployed to the Tibetan plateau at 5,250m asl. AliCPT-1 is a 95/150GHz 72cm aperture, two lens refracting telescope cooled down to 4K. Alumina lenses image the CMB on a 636mm wide focal plane. 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The design of the Ali CMB Polarization Telescope receiver
AliCPT-1 is the first CMB degree scale polarimeter to be deployed to the Tibetan plateau at 5,250m asl. AliCPT-1 is a 95/150GHz 72cm aperture, two lens refracting telescope cooled down to 4K. Alumina lenses image the CMB on a 636mm wide focal plane. The modularized focal plane consists of dichroic polarization-sensitive Transition-Edge Sensors (TESes). Each module includes 1,704 optically active TESes fabricated on a 6in Silicon wafer. Each TES array is read out with a microwave multiplexing with a multiplexing factor up to 2,000. Such large factor has allowed to consider 10's of thousands of detectors in a practical way, enabling to design a receiver that can operate up to 19 TES arrays for a total of 32,300 TESes. AliCPT-1 leverages the technological advancements of AdvACT and BICEP-3. The cryostat receiver is currently under integration and testing. Here we present the AliCPT-1 receiver, underlying how the optimized design meets the experimental requirements.
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