The performance of SiPM-based gamma-ray detector (GRD) of GECAM-C
As a new member of GECAM mission, the GECAM-C (also called High Energy Burst Searcher, HEBS) is a gamma-ray all-sky monitor onboard SATech-01 satellite, which was launched on July 27th, 2022 to detect gamma-ray transients from 6 keV to 6 MeV, such as Gamma-Ray Bursts (GRBs), high energy counterpart...
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creator | Zhang, Dali Zheng, Chao Liu, Jiacong An, Zhenghua Wang, Chenwei Wen, Xiangyang Li, Xinqiao Sun, Xilei Gong, Ke Liu, Yaqing Liu, Xiaojing Yang, Sheng Peng, Wenxi Qiao, Rui Guo, Dongya Feng, Peiyi Zhang, Yanqiu Xue, Wangchen Tan, Wenjun Cai, Ce Xiao, Shuo Yi, Qibin Xu, Yanbing Gao, Min Wang, Jinzhou Hou, Dongjie Huang, Yue Zhao, Xiaoyun Ma, Xiang Wang, Ping Wang, Jin Li, Xiaobo Zhang, Peng Zhang, Zhen Li, Yanguo Wang, Hui Liang, Xiaohua Wang, Yuxi Li, Bing Ye, Jianying Zheng, Shijie Song, Liming Zhang, Fan Chen, Gang Xiong, Shaolin |
description | As a new member of GECAM mission, the GECAM-C (also called High Energy Burst Searcher, HEBS) is a gamma-ray all-sky monitor onboard SATech-01 satellite, which was launched on July 27th, 2022 to detect gamma-ray transients from 6 keV to 6 MeV, such as Gamma-Ray Bursts (GRBs), high energy counterpart of Gravitational Waves (GWs) and Fast Radio Bursts (FRBs), and Soft Gamma-ray Repeaters (SGRs). Together with GECAM-A and GECAM-B launched in December 2020, GECAM-C will greatly improve the monitoring coverage, localization, as well as temporal and spectral measurements of gamma-ray transients. GECAM-C employs 12 SiPM-based Gamma-Ray Detectors (GRDs) to detect gamma-ray transients . In this paper, we firstly give a brief description of the design of GECAM-C GRDs, and then focus on the on-ground tests and in-flight performance of GRDs. We also did the comparison study of the SiPM in-flight performance between GECAM-C and GECAM-B. The results show GECAM-C GRD works as expected and is ready to make scientific observations. |
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Together with GECAM-A and GECAM-B launched in December 2020, GECAM-C will greatly improve the monitoring coverage, localization, as well as temporal and spectral measurements of gamma-ray transients. GECAM-C employs 12 SiPM-based Gamma-Ray Detectors (GRDs) to detect gamma-ray transients . In this paper, we firstly give a brief description of the design of GECAM-C GRDs, and then focus on the on-ground tests and in-flight performance of GRDs. We also did the comparison study of the SiPM in-flight performance between GECAM-C and GECAM-B. The results show GECAM-C GRD works as expected and is ready to make scientific observations.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Flight characteristics ; Gamma ray bursts ; Gamma ray detectors ; Gravitational waves ; Ground tests ; Radio bursts ; Repeaters</subject><ispartof>arXiv.org, 2023-03</ispartof><rights>2023. This work is published under http://creativecommons.org/licenses/by-nc-nd/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>777,781</link.rule.ids></links><search><creatorcontrib>Zhang, Dali</creatorcontrib><creatorcontrib>Zheng, Chao</creatorcontrib><creatorcontrib>Liu, Jiacong</creatorcontrib><creatorcontrib>An, Zhenghua</creatorcontrib><creatorcontrib>Wang, Chenwei</creatorcontrib><creatorcontrib>Wen, Xiangyang</creatorcontrib><creatorcontrib>Li, Xinqiao</creatorcontrib><creatorcontrib>Sun, Xilei</creatorcontrib><creatorcontrib>Gong, Ke</creatorcontrib><creatorcontrib>Liu, Yaqing</creatorcontrib><creatorcontrib>Liu, Xiaojing</creatorcontrib><creatorcontrib>Yang, Sheng</creatorcontrib><creatorcontrib>Peng, Wenxi</creatorcontrib><creatorcontrib>Qiao, Rui</creatorcontrib><creatorcontrib>Guo, Dongya</creatorcontrib><creatorcontrib>Feng, Peiyi</creatorcontrib><creatorcontrib>Zhang, Yanqiu</creatorcontrib><creatorcontrib>Xue, Wangchen</creatorcontrib><creatorcontrib>Tan, Wenjun</creatorcontrib><creatorcontrib>Cai, Ce</creatorcontrib><creatorcontrib>Xiao, Shuo</creatorcontrib><creatorcontrib>Yi, Qibin</creatorcontrib><creatorcontrib>Xu, Yanbing</creatorcontrib><creatorcontrib>Gao, Min</creatorcontrib><creatorcontrib>Wang, Jinzhou</creatorcontrib><creatorcontrib>Hou, Dongjie</creatorcontrib><creatorcontrib>Huang, Yue</creatorcontrib><creatorcontrib>Zhao, Xiaoyun</creatorcontrib><creatorcontrib>Ma, Xiang</creatorcontrib><creatorcontrib>Wang, Ping</creatorcontrib><creatorcontrib>Wang, Jin</creatorcontrib><creatorcontrib>Li, Xiaobo</creatorcontrib><creatorcontrib>Zhang, Peng</creatorcontrib><creatorcontrib>Zhang, Zhen</creatorcontrib><creatorcontrib>Li, Yanguo</creatorcontrib><creatorcontrib>Wang, Hui</creatorcontrib><creatorcontrib>Liang, Xiaohua</creatorcontrib><creatorcontrib>Wang, Yuxi</creatorcontrib><creatorcontrib>Li, Bing</creatorcontrib><creatorcontrib>Ye, Jianying</creatorcontrib><creatorcontrib>Zheng, Shijie</creatorcontrib><creatorcontrib>Song, Liming</creatorcontrib><creatorcontrib>Zhang, Fan</creatorcontrib><creatorcontrib>Chen, Gang</creatorcontrib><creatorcontrib>Xiong, Shaolin</creatorcontrib><title>The performance of SiPM-based gamma-ray detector (GRD) of GECAM-C</title><title>arXiv.org</title><description>As a new member of GECAM mission, the GECAM-C (also called High Energy Burst Searcher, HEBS) is a gamma-ray all-sky monitor onboard SATech-01 satellite, which was launched on July 27th, 2022 to detect gamma-ray transients from 6 keV to 6 MeV, such as Gamma-Ray Bursts (GRBs), high energy counterpart of Gravitational Waves (GWs) and Fast Radio Bursts (FRBs), and Soft Gamma-ray Repeaters (SGRs). Together with GECAM-A and GECAM-B launched in December 2020, GECAM-C will greatly improve the monitoring coverage, localization, as well as temporal and spectral measurements of gamma-ray transients. GECAM-C employs 12 SiPM-based Gamma-Ray Detectors (GRDs) to detect gamma-ray transients . In this paper, we firstly give a brief description of the design of GECAM-C GRDs, and then focus on the on-ground tests and in-flight performance of GRDs. We also did the comparison study of the SiPM in-flight performance between GECAM-C and GECAM-B. The results show GECAM-C GRD works as expected and is ready to make scientific observations.</description><subject>Flight characteristics</subject><subject>Gamma ray bursts</subject><subject>Gamma ray detectors</subject><subject>Gravitational waves</subject><subject>Ground tests</subject><subject>Radio bursts</subject><subject>Repeaters</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNpjYuA0MjY21LUwMTLiYOAtLs4yMDAwMjM3MjU15mRwDMlIVShILUrLL8pNzEtOVchPUwjODPDVTUosTk1RSE_MzU3ULUqsVEhJLUlNLskvUtBwD3LRBClzd3V29NV15mFgTUvMKU7lhdLcDMpuriHOHroFRfmFpanFJfFZ-aVFeUCpeCNzC0MTQ0MTM1Nj4lQBAFuiNsc</recordid><startdate>20230307</startdate><enddate>20230307</enddate><creator>Zhang, Dali</creator><creator>Zheng, Chao</creator><creator>Liu, 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Shaolin</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central 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Shijie</au><au>Song, Liming</au><au>Zhang, Fan</au><au>Chen, Gang</au><au>Xiong, Shaolin</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>The performance of SiPM-based gamma-ray detector (GRD) of GECAM-C</atitle><jtitle>arXiv.org</jtitle><date>2023-03-07</date><risdate>2023</risdate><eissn>2331-8422</eissn><abstract>As a new member of GECAM mission, the GECAM-C (also called High Energy Burst Searcher, HEBS) is a gamma-ray all-sky monitor onboard SATech-01 satellite, which was launched on July 27th, 2022 to detect gamma-ray transients from 6 keV to 6 MeV, such as Gamma-Ray Bursts (GRBs), high energy counterpart of Gravitational Waves (GWs) and Fast Radio Bursts (FRBs), and Soft Gamma-ray Repeaters (SGRs). Together with GECAM-A and GECAM-B launched in December 2020, GECAM-C will greatly improve the monitoring coverage, localization, as well as temporal and spectral measurements of gamma-ray transients. GECAM-C employs 12 SiPM-based Gamma-Ray Detectors (GRDs) to detect gamma-ray transients . In this paper, we firstly give a brief description of the design of GECAM-C GRDs, and then focus on the on-ground tests and in-flight performance of GRDs. We also did the comparison study of the SiPM in-flight performance between GECAM-C and GECAM-B. The results show GECAM-C GRD works as expected and is ready to make scientific observations.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
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subjects | Flight characteristics Gamma ray bursts Gamma ray detectors Gravitational waves Ground tests Radio bursts Repeaters |
title | The performance of SiPM-based gamma-ray detector (GRD) of GECAM-C |
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