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. |
| doi_str_mv | 10.48550/arxiv.2303.00537 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2303_00537</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2303_00537</sourcerecordid><originalsourceid>FETCH-LOGICAL-a677-1a140c0fb236f9369434a5cacf2234a3eb728bcddaf5108416f44234bf651383</originalsourceid><addsrcrecordid>eNotj7FuwjAURb0wVNAP6FSPMDi1_WwnjFFKUyRQK2CPnh0_GqlpkEFV-fsC7XSvdI-udBh7UDIzhbXyCdNP951pkJBJaSG_Y-XuI_JDTDSkHr9C5APxbfe-Fh6PseV77HsUCc-8jacYTkPi03rzPLti9aIq16KasBHh5zHe_-eYbV8Wu-pVrN7qZVWuBLo8FwqVkUGS1-BoDm5uwKANGEjrS4Poc1340LZIVsnCKEfGXBZPziooYMwe_15vCs0hdT2mc3NVaW4q8At1Q0C_</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>The performance of SiPM-based gamma-ray detector (GRD) of GECAM-C</title><source>arXiv.org</source><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</creator><creatorcontrib>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</creatorcontrib><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><identifier>DOI: 10.48550/arxiv.2303.00537</identifier><language>eng</language><subject>Physics - Instrumentation and Detectors ; Physics - Instrumentation and Methods for Astrophysics</subject><creationdate>2023-03</creationdate><rights>http://creativecommons.org/licenses/by-nc-nd/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2303.00537$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2303.00537$$DView paper in arXiv$$Hfree_for_read</backlink></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><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>Physics - Instrumentation and Detectors</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj7FuwjAURb0wVNAP6FSPMDi1_WwnjFFKUyRQK2CPnh0_GqlpkEFV-fsC7XSvdI-udBh7UDIzhbXyCdNP951pkJBJaSG_Y-XuI_JDTDSkHr9C5APxbfe-Fh6PseV77HsUCc-8jacYTkPi03rzPLti9aIq16KasBHh5zHe_-eYbV8Wu-pVrN7qZVWuBLo8FwqVkUGS1-BoDm5uwKANGEjrS4Poc1340LZIVsnCKEfGXBZPziooYMwe_15vCs0hdT2mc3NVaW4q8At1Q0C_</recordid><startdate>20230301</startdate><enddate>20230301</enddate><creator>Zhang, Dali</creator><creator>Zheng, Chao</creator><creator>Liu, Jiacong</creator><creator>An, Zhenghua</creator><creator>Wang, Chenwei</creator><creator>Wen, Xiangyang</creator><creator>Li, Xinqiao</creator><creator>Sun, Xilei</creator><creator>Gong, Ke</creator><creator>Liu, Yaqing</creator><creator>Liu, Xiaojing</creator><creator>Yang, Sheng</creator><creator>Peng, Wenxi</creator><creator>Qiao, Rui</creator><creator>Guo, Dongya</creator><creator>Feng, Peiyi</creator><creator>Zhang, Yanqiu</creator><creator>Xue, Wangchen</creator><creator>Tan, Wenjun</creator><creator>Cai, Ce</creator><creator>Xiao, Shuo</creator><creator>Yi, Qibin</creator><creator>Xu, Yanbing</creator><creator>Gao, Min</creator><creator>Wang, Jinzhou</creator><creator>Hou, Dongjie</creator><creator>Huang, Yue</creator><creator>Zhao, Xiaoyun</creator><creator>Ma, Xiang</creator><creator>Wang, Ping</creator><creator>Wang, Jin</creator><creator>Li, Xiaobo</creator><creator>Zhang, Peng</creator><creator>Zhang, Zhen</creator><creator>Li, Yanguo</creator><creator>Wang, Hui</creator><creator>Liang, Xiaohua</creator><creator>Wang, Yuxi</creator><creator>Li, Bing</creator><creator>Ye, Jianying</creator><creator>Zheng, Shijie</creator><creator>Song, Liming</creator><creator>Zhang, Fan</creator><creator>Chen, Gang</creator><creator>Xiong, Shaolin</creator><scope>GOX</scope></search><sort><creationdate>20230301</creationdate><title>The performance of SiPM-based gamma-ray detector (GRD) of GECAM-C</title><author>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</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a677-1a140c0fb236f9369434a5cacf2234a3eb728bcddaf5108416f44234bf651383</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Physics - Instrumentation and Detectors</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><toplevel>online_resources</toplevel><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><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Zhang, Dali</au><au>Zheng, Chao</au><au>Liu, Jiacong</au><au>An, Zhenghua</au><au>Wang, Chenwei</au><au>Wen, Xiangyang</au><au>Li, Xinqiao</au><au>Sun, Xilei</au><au>Gong, Ke</au><au>Liu, Yaqing</au><au>Liu, Xiaojing</au><au>Yang, Sheng</au><au>Peng, Wenxi</au><au>Qiao, Rui</au><au>Guo, Dongya</au><au>Feng, Peiyi</au><au>Zhang, Yanqiu</au><au>Xue, Wangchen</au><au>Tan, Wenjun</au><au>Cai, Ce</au><au>Xiao, Shuo</au><au>Yi, Qibin</au><au>Xu, Yanbing</au><au>Gao, Min</au><au>Wang, Jinzhou</au><au>Hou, Dongjie</au><au>Huang, Yue</au><au>Zhao, Xiaoyun</au><au>Ma, Xiang</au><au>Wang, Ping</au><au>Wang, Jin</au><au>Li, Xiaobo</au><au>Zhang, Peng</au><au>Zhang, Zhen</au><au>Li, Yanguo</au><au>Wang, Hui</au><au>Liang, Xiaohua</au><au>Wang, Yuxi</au><au>Li, Bing</au><au>Ye, Jianying</au><au>Zheng, Shijie</au><au>Song, Liming</au><au>Zhang, Fan</au><au>Chen, Gang</au><au>Xiong, Shaolin</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The performance of SiPM-based gamma-ray detector (GRD) of GECAM-C</atitle><date>2023-03-01</date><risdate>2023</risdate><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><doi>10.48550/arxiv.2303.00537</doi><oa>free_for_read</oa></addata></record> |
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| identifier | DOI: 10.48550/arxiv.2303.00537 |
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| subjects | Physics - Instrumentation and Detectors Physics - Instrumentation and Methods for Astrophysics |
| title | The performance of SiPM-based gamma-ray detector (GRD) of GECAM-C |
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