Energetic transients joint analysis system for multi-INstrument (ETJASMIN) for GECAM – I. Positional, temporal, and spectral analyses

ABSTRACT Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a dedicated mission, launched in December 2020, for gamma-ray transients, including gamma-ray bursts (GRBs) and soft gamma repeater (SGR) bursts in the multimessenger and multiwavelength astronomy era. Sin...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2022-06, Vol.514 (2), p.2397-2406
Hauptverfasser: Xiao, Shuo, Xiong, Shao-Lin, Cai, Ce, Song, Li-Ming, Zheng, Shi-Jie, Peng, Wen-Xi, Wang, Ping, Qiao, Rui, Guo, Dong-Ya, Wang, Jin, Li, Xiao-Bo, Song, Xin-Ying, Yuan, Yong, Fan, Xi-Long, Zhao, Xiao-Yun, Huang, Yue, Ma, Xiang, Zhang, Peng, Li, Bing, Ge, Ming-Yu, Tuo, You-Li, Chen, Wei, Zhang, Hong-Mei, He, Jian-Jian, Li, Chao-Yang, Yi, Qi-Bin, Zhao, Yi, Zhang, Yan-Qiu, Zheng, Chao, Xue, Wang-Chen, Liu, Jia-Cong, Zhang, Zhen, Li, Cheng-Kui, Zhang, Xiao-Lu, Zhao, Hong-Yu, Zhao, Guo-Ying, Guo, Zhi-Wei, Xie, Sheng-Lun, Wang, Chen-Wei, Zhang, Bo-Xin, Wang, Yue, Li, Qing-Xin, Li, Chao, Zhang, Kai, Shi, Dong-Li, Zhao, Shi-Yi, Yao, Min, An, Zheng-Hua, Chen, Chan, Gong, Ke, Liu, Ya-Qing, Gao, Min, Li, Xin-Qiao, Li, Yan-Guo, Liang, Xiao-Hua, Liu, Xiao-Jing, Sun, Xi-Lei, Wang, Jin-Zhou, Wen, Xiang-Yang, Xu, Yan-Bing, Xu, Yu-Peng, Yang, Sheng, Zhang, Chao-Yue, Zhang, Da-Li, Zhang, Fei, Chen, Gang, Lu, Fang-Jun, Sun, Gong-Xing, Zhang, Fan, Zhang, Shuang-Nan
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creator Xiao, Shuo
Xiong, Shao-Lin
Cai, Ce
Song, Li-Ming
Zheng, Shi-Jie
Peng, Wen-Xi
Wang, Ping
Qiao, Rui
Guo, Dong-Ya
Wang, Jin
Li, Xiao-Bo
Song, Xin-Ying
Yuan, Yong
Fan, Xi-Long
Zhao, Xiao-Yun
Huang, Yue
Ma, Xiang
Zhang, Peng
Li, Bing
Ge, Ming-Yu
Tuo, You-Li
Chen, Wei
Zhang, Hong-Mei
He, Jian-Jian
Li, Chao-Yang
Yi, Qi-Bin
Zhao, Yi
Zhang, Yan-Qiu
Zheng, Chao
Xue, Wang-Chen
Liu, Jia-Cong
Zhang, Zhen
Li, Cheng-Kui
Zhang, Xiao-Lu
Zhao, Hong-Yu
Zhao, Guo-Ying
Guo, Zhi-Wei
Xie, Sheng-Lun
Wang, Chen-Wei
Zhang, Bo-Xin
Wang, Yue
Li, Qing-Xin
Li, Chao
Zhang, Kai
Shi, Dong-Li
Zhao, Shi-Yi
Yao, Min
An, Zheng-Hua
Chen, Chan
Gong, Ke
Liu, Ya-Qing
Gao, Min
Li, Xin-Qiao
Li, Yan-Guo
Liang, Xiao-Hua
Liu, Xiao-Jing
Sun, Xi-Lei
Wang, Jin-Zhou
Wen, Xiang-Yang
Xu, Yan-Bing
Xu, Yu-Peng
Yang, Sheng
Zhang, Chao-Yue
Zhang, Da-Li
Zhang, Fei
Chen, Gang
Lu, Fang-Jun
Sun, Gong-Xing
Zhang, Fan
Zhang, Shuang-Nan
description ABSTRACT Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a dedicated mission, launched in December 2020, for gamma-ray transients, including gamma-ray bursts (GRBs) and soft gamma repeater (SGR) bursts in the multimessenger and multiwavelength astronomy era. Since GECAM consists of two independent spacecrafts (or say instruments), and the framework of data analysis for multiple spacecrafts is distinctive from that for only one spacecraft, which is the case for most GRB missions, we developed a dedicated pipeline called Energetic Transients Joint Analysis System for Multi-INstrument (ETJASMIN) for GECAM mission. This pipeline has been naturally extended to incorporate data from other gamma-ray instruments, including the operating missions, such as Insight-HXMT/HE, Fermi/GBM, Swift/BAT, INTEGRAL/SPI-ACS, Konus-Wind, and GRID, as well as the forthcoming missions, such as SVOM/GRM and HEBS. In this paper, we present this pipeline with a focus on the data analysis procedures, methodology, and results in terms of the localization, verification (classification), spectral, and temporal analyses of gamma-ray transients. We show that this pipeline could provide more accurate, reliable, and comprehensive results than that of individual spacecraft, which is beneficial for gamma-ray transients observation.
doi_str_mv 10.1093/mnras/stac999
format Article
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Positional, temporal, and spectral analyses</title><source>Oxford Journals Open Access Collection</source><creator>Xiao, Shuo ; Xiong, Shao-Lin ; Cai, Ce ; Song, Li-Ming ; Zheng, Shi-Jie ; Peng, Wen-Xi ; Wang, Ping ; Qiao, Rui ; Guo, Dong-Ya ; Wang, Jin ; Li, Xiao-Bo ; Song, Xin-Ying ; Yuan, Yong ; Fan, Xi-Long ; Zhao, Xiao-Yun ; Huang, Yue ; Ma, Xiang ; Zhang, Peng ; Li, Bing ; Ge, Ming-Yu ; Tuo, You-Li ; Chen, Wei ; Zhang, Hong-Mei ; He, Jian-Jian ; Li, Chao-Yang ; Yi, Qi-Bin ; Zhao, Yi ; Zhang, Yan-Qiu ; Zheng, Chao ; Xue, Wang-Chen ; Liu, Jia-Cong ; Zhang, Zhen ; Li, Cheng-Kui ; Zhang, Xiao-Lu ; Zhao, Hong-Yu ; Zhao, Guo-Ying ; Guo, Zhi-Wei ; Xie, Sheng-Lun ; Wang, Chen-Wei ; Zhang, Bo-Xin ; Wang, Yue ; Li, Qing-Xin ; Li, Chao ; Zhang, Kai ; Shi, Dong-Li ; Zhao, Shi-Yi ; Yao, Min ; An, Zheng-Hua ; Chen, Chan ; Gong, Ke ; Liu, Ya-Qing ; Gao, Min ; Li, Xin-Qiao ; Li, Yan-Guo ; Liang, Xiao-Hua ; Liu, Xiao-Jing ; Sun, Xi-Lei ; Wang, Jin-Zhou ; Wen, Xiang-Yang ; Xu, Yan-Bing ; Xu, Yu-Peng ; Yang, Sheng ; Zhang, Chao-Yue ; Zhang, Da-Li ; Zhang, Fei ; Chen, Gang ; Lu, Fang-Jun ; Sun, Gong-Xing ; Zhang, Fan ; Zhang, Shuang-Nan</creator><creatorcontrib>Xiao, Shuo ; Xiong, Shao-Lin ; Cai, Ce ; Song, Li-Ming ; Zheng, Shi-Jie ; Peng, Wen-Xi ; Wang, Ping ; Qiao, Rui ; Guo, Dong-Ya ; Wang, Jin ; Li, Xiao-Bo ; Song, Xin-Ying ; Yuan, Yong ; Fan, Xi-Long ; Zhao, Xiao-Yun ; Huang, Yue ; Ma, Xiang ; Zhang, Peng ; Li, Bing ; Ge, Ming-Yu ; Tuo, You-Li ; Chen, Wei ; Zhang, Hong-Mei ; He, Jian-Jian ; Li, Chao-Yang ; Yi, Qi-Bin ; Zhao, Yi ; Zhang, Yan-Qiu ; Zheng, Chao ; Xue, Wang-Chen ; Liu, Jia-Cong ; Zhang, Zhen ; Li, Cheng-Kui ; Zhang, Xiao-Lu ; Zhao, Hong-Yu ; Zhao, Guo-Ying ; Guo, Zhi-Wei ; Xie, Sheng-Lun ; Wang, Chen-Wei ; Zhang, Bo-Xin ; Wang, Yue ; Li, Qing-Xin ; Li, Chao ; Zhang, Kai ; Shi, Dong-Li ; Zhao, Shi-Yi ; Yao, Min ; An, Zheng-Hua ; Chen, Chan ; Gong, Ke ; Liu, Ya-Qing ; Gao, Min ; Li, Xin-Qiao ; Li, Yan-Guo ; Liang, Xiao-Hua ; Liu, Xiao-Jing ; Sun, Xi-Lei ; Wang, Jin-Zhou ; Wen, Xiang-Yang ; Xu, Yan-Bing ; Xu, Yu-Peng ; Yang, Sheng ; Zhang, Chao-Yue ; Zhang, Da-Li ; Zhang, Fei ; Chen, Gang ; Lu, Fang-Jun ; Sun, Gong-Xing ; Zhang, Fan ; Zhang, Shuang-Nan</creatorcontrib><description>ABSTRACT Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a dedicated mission, launched in December 2020, for gamma-ray transients, including gamma-ray bursts (GRBs) and soft gamma repeater (SGR) bursts in the multimessenger and multiwavelength astronomy era. Since GECAM consists of two independent spacecrafts (or say instruments), and the framework of data analysis for multiple spacecrafts is distinctive from that for only one spacecraft, which is the case for most GRB missions, we developed a dedicated pipeline called Energetic Transients Joint Analysis System for Multi-INstrument (ETJASMIN) for GECAM mission. This pipeline has been naturally extended to incorporate data from other gamma-ray instruments, including the operating missions, such as Insight-HXMT/HE, Fermi/GBM, Swift/BAT, INTEGRAL/SPI-ACS, Konus-Wind, and GRID, as well as the forthcoming missions, such as SVOM/GRM and HEBS. In this paper, we present this pipeline with a focus on the data analysis procedures, methodology, and results in terms of the localization, verification (classification), spectral, and temporal analyses of gamma-ray transients. 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Positional, temporal, and spectral analyses</title><title>Monthly notices of the Royal Astronomical Society</title><description>ABSTRACT Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a dedicated mission, launched in December 2020, for gamma-ray transients, including gamma-ray bursts (GRBs) and soft gamma repeater (SGR) bursts in the multimessenger and multiwavelength astronomy era. Since GECAM consists of two independent spacecrafts (or say instruments), and the framework of data analysis for multiple spacecrafts is distinctive from that for only one spacecraft, which is the case for most GRB missions, we developed a dedicated pipeline called Energetic Transients Joint Analysis System for Multi-INstrument (ETJASMIN) for GECAM mission. This pipeline has been naturally extended to incorporate data from other gamma-ray instruments, including the operating missions, such as Insight-HXMT/HE, Fermi/GBM, Swift/BAT, INTEGRAL/SPI-ACS, Konus-Wind, and GRID, as well as the forthcoming missions, such as SVOM/GRM and HEBS. In this paper, we present this pipeline with a focus on the data analysis procedures, methodology, and results in terms of the localization, verification (classification), spectral, and temporal analyses of gamma-ray transients. 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Shi-Jie</au><au>Peng, Wen-Xi</au><au>Wang, Ping</au><au>Qiao, Rui</au><au>Guo, Dong-Ya</au><au>Wang, Jin</au><au>Li, Xiao-Bo</au><au>Song, Xin-Ying</au><au>Yuan, Yong</au><au>Fan, Xi-Long</au><au>Zhao, Xiao-Yun</au><au>Huang, Yue</au><au>Ma, Xiang</au><au>Zhang, Peng</au><au>Li, Bing</au><au>Ge, Ming-Yu</au><au>Tuo, You-Li</au><au>Chen, Wei</au><au>Zhang, Hong-Mei</au><au>He, Jian-Jian</au><au>Li, Chao-Yang</au><au>Yi, Qi-Bin</au><au>Zhao, Yi</au><au>Zhang, Yan-Qiu</au><au>Zheng, Chao</au><au>Xue, Wang-Chen</au><au>Liu, Jia-Cong</au><au>Zhang, Zhen</au><au>Li, Cheng-Kui</au><au>Zhang, Xiao-Lu</au><au>Zhao, Hong-Yu</au><au>Zhao, Guo-Ying</au><au>Guo, Zhi-Wei</au><au>Xie, Sheng-Lun</au><au>Wang, Chen-Wei</au><au>Zhang, Bo-Xin</au><au>Wang, Yue</au><au>Li, Qing-Xin</au><au>Li, Chao</au><au>Zhang, Kai</au><au>Shi, Dong-Li</au><au>Zhao, Shi-Yi</au><au>Yao, Min</au><au>An, Zheng-Hua</au><au>Chen, Chan</au><au>Gong, Ke</au><au>Liu, Ya-Qing</au><au>Gao, Min</au><au>Li, Xin-Qiao</au><au>Li, Yan-Guo</au><au>Liang, Xiao-Hua</au><au>Liu, Xiao-Jing</au><au>Sun, Xi-Lei</au><au>Wang, Jin-Zhou</au><au>Wen, Xiang-Yang</au><au>Xu, Yan-Bing</au><au>Xu, Yu-Peng</au><au>Yang, Sheng</au><au>Zhang, Chao-Yue</au><au>Zhang, Da-Li</au><au>Zhang, Fei</au><au>Chen, Gang</au><au>Lu, Fang-Jun</au><au>Sun, Gong-Xing</au><au>Zhang, Fan</au><au>Zhang, Shuang-Nan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Energetic transients joint analysis system for multi-INstrument (ETJASMIN) for GECAM – I. Positional, temporal, and spectral analyses</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>2022-06-17</date><risdate>2022</risdate><volume>514</volume><issue>2</issue><spage>2397</spage><epage>2406</epage><pages>2397-2406</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>ABSTRACT Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a dedicated mission, launched in December 2020, for gamma-ray transients, including gamma-ray bursts (GRBs) and soft gamma repeater (SGR) bursts in the multimessenger and multiwavelength astronomy era. Since GECAM consists of two independent spacecrafts (or say instruments), and the framework of data analysis for multiple spacecrafts is distinctive from that for only one spacecraft, which is the case for most GRB missions, we developed a dedicated pipeline called Energetic Transients Joint Analysis System for Multi-INstrument (ETJASMIN) for GECAM mission. This pipeline has been naturally extended to incorporate data from other gamma-ray instruments, including the operating missions, such as Insight-HXMT/HE, Fermi/GBM, Swift/BAT, INTEGRAL/SPI-ACS, Konus-Wind, and GRID, as well as the forthcoming missions, such as SVOM/GRM and HEBS. In this paper, we present this pipeline with a focus on the data analysis procedures, methodology, and results in terms of the localization, verification (classification), spectral, and temporal analyses of gamma-ray transients. We show that this pipeline could provide more accurate, reliable, and comprehensive results than that of individual spacecraft, which is beneficial for gamma-ray transients observation.</abstract><pub>Oxford University Press</pub><doi>10.1093/mnras/stac999</doi><tpages>10</tpages><orcidid>https://orcid.org/0000-0003-2957-2806</orcidid><orcidid>https://orcid.org/0000-0002-2176-8778</orcidid><orcidid>https://orcid.org/0000-0003-0274-3396</orcidid><orcidid>https://orcid.org/0000-0002-8174-0128</orcidid><oa>free_for_read</oa></addata></record>
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title Energetic transients joint analysis system for multi-INstrument (ETJASMIN) for GECAM – I. Positional, temporal, and spectral analyses
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