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 |
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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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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.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/stac999</identifier><language>eng</language><publisher>Oxford University Press</publisher><ispartof>Monthly notices of the Royal Astronomical Society, 2022-06, Vol.514 (2), p.2397-2406</ispartof><rights>2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society 2022</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c309t-6eedca1bab0a4ea126c0ef0829bdf5caf07f06455e86443319e9402db677c8b83</citedby><cites>FETCH-LOGICAL-c309t-6eedca1bab0a4ea126c0ef0829bdf5caf07f06455e86443319e9402db677c8b83</cites><orcidid>0000-0003-2957-2806 ; 0000-0002-2176-8778 ; 0000-0003-0274-3396 ; 0000-0002-8174-0128</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,1598,27903,27904</link.rule.ids></links><search><creatorcontrib>Xiao, Shuo</creatorcontrib><creatorcontrib>Xiong, Shao-Lin</creatorcontrib><creatorcontrib>Cai, Ce</creatorcontrib><creatorcontrib>Song, Li-Ming</creatorcontrib><creatorcontrib>Zheng, Shi-Jie</creatorcontrib><creatorcontrib>Peng, Wen-Xi</creatorcontrib><creatorcontrib>Wang, Ping</creatorcontrib><creatorcontrib>Qiao, Rui</creatorcontrib><creatorcontrib>Guo, Dong-Ya</creatorcontrib><creatorcontrib>Wang, Jin</creatorcontrib><creatorcontrib>Li, Xiao-Bo</creatorcontrib><creatorcontrib>Song, Xin-Ying</creatorcontrib><creatorcontrib>Yuan, Yong</creatorcontrib><creatorcontrib>Fan, Xi-Long</creatorcontrib><creatorcontrib>Zhao, Xiao-Yun</creatorcontrib><creatorcontrib>Huang, Yue</creatorcontrib><creatorcontrib>Ma, Xiang</creatorcontrib><creatorcontrib>Zhang, Peng</creatorcontrib><creatorcontrib>Li, Bing</creatorcontrib><creatorcontrib>Ge, Ming-Yu</creatorcontrib><creatorcontrib>Tuo, You-Li</creatorcontrib><creatorcontrib>Chen, Wei</creatorcontrib><creatorcontrib>Zhang, Hong-Mei</creatorcontrib><creatorcontrib>He, Jian-Jian</creatorcontrib><creatorcontrib>Li, Chao-Yang</creatorcontrib><creatorcontrib>Yi, Qi-Bin</creatorcontrib><creatorcontrib>Zhao, Yi</creatorcontrib><creatorcontrib>Zhang, Yan-Qiu</creatorcontrib><creatorcontrib>Zheng, Chao</creatorcontrib><creatorcontrib>Xue, Wang-Chen</creatorcontrib><creatorcontrib>Liu, Jia-Cong</creatorcontrib><creatorcontrib>Zhang, Zhen</creatorcontrib><creatorcontrib>Li, Cheng-Kui</creatorcontrib><creatorcontrib>Zhang, Xiao-Lu</creatorcontrib><creatorcontrib>Zhao, Hong-Yu</creatorcontrib><creatorcontrib>Zhao, Guo-Ying</creatorcontrib><creatorcontrib>Guo, Zhi-Wei</creatorcontrib><creatorcontrib>Xie, Sheng-Lun</creatorcontrib><creatorcontrib>Wang, Chen-Wei</creatorcontrib><creatorcontrib>Zhang, Bo-Xin</creatorcontrib><creatorcontrib>Wang, Yue</creatorcontrib><creatorcontrib>Li, Qing-Xin</creatorcontrib><creatorcontrib>Li, Chao</creatorcontrib><creatorcontrib>Zhang, Kai</creatorcontrib><creatorcontrib>Shi, Dong-Li</creatorcontrib><creatorcontrib>Zhao, Shi-Yi</creatorcontrib><creatorcontrib>Yao, Min</creatorcontrib><creatorcontrib>An, Zheng-Hua</creatorcontrib><creatorcontrib>Chen, Chan</creatorcontrib><creatorcontrib>Gong, Ke</creatorcontrib><creatorcontrib>Liu, Ya-Qing</creatorcontrib><creatorcontrib>Gao, Min</creatorcontrib><creatorcontrib>Li, Xin-Qiao</creatorcontrib><creatorcontrib>Li, Yan-Guo</creatorcontrib><creatorcontrib>Liang, Xiao-Hua</creatorcontrib><creatorcontrib>Liu, Xiao-Jing</creatorcontrib><creatorcontrib>Sun, Xi-Lei</creatorcontrib><creatorcontrib>Wang, Jin-Zhou</creatorcontrib><creatorcontrib>Wen, Xiang-Yang</creatorcontrib><creatorcontrib>Xu, Yan-Bing</creatorcontrib><creatorcontrib>Xu, Yu-Peng</creatorcontrib><creatorcontrib>Yang, Sheng</creatorcontrib><creatorcontrib>Zhang, Chao-Yue</creatorcontrib><creatorcontrib>Zhang, Da-Li</creatorcontrib><creatorcontrib>Zhang, Fei</creatorcontrib><creatorcontrib>Chen, Gang</creatorcontrib><creatorcontrib>Lu, Fang-Jun</creatorcontrib><creatorcontrib>Sun, Gong-Xing</creatorcontrib><creatorcontrib>Zhang, Fan</creatorcontrib><creatorcontrib>Zhang, Shuang-Nan</creatorcontrib><title>Energetic transients joint analysis system for multi-INstrument (ETJASMIN) for GECAM – I. 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. 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.</description><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>TOX</sourceid><recordid>eNqFkL1OwzAUhS0EEqUwsnssEmntOHHisapCCWoLEmWOHMdBrvInX3fIxsYD8IY8CenPznSPdD99RzoI3VMypUSwWd1YCTNwUgkhLtCIMh56vuD8Eo0IYaEXR5ReoxuAHSEkYD4foe-k0fZTO6Ows7IBoxsHeNeaxmHZyKoHAxh6cLrGZWtxva-c8dINOLuvBxZPku3L_H2dbh6O_2WymK_x79cPTqf4rQXjTDtoHvEg6Fp7SLIpMHRaDX3VuUPDLboqZQX67nzH6OMp2S6evdXrMl3MV55iRDiPa10oSXOZExloSX2uiC5J7Iu8KEMlSxKVhAdhqGMeBIxRoUVA_CLnUaTiPGZj5J28yrYAVpdZZ00tbZ9Rkh1WzI4rZucVB35y4tt99w_6B8MteJQ</recordid><startdate>20220617</startdate><enddate>20220617</enddate><creator>Xiao, Shuo</creator><creator>Xiong, Shao-Lin</creator><creator>Cai, Ce</creator><creator>Song, Li-Ming</creator><creator>Zheng, Shi-Jie</creator><creator>Peng, Wen-Xi</creator><creator>Wang, Ping</creator><creator>Qiao, Rui</creator><creator>Guo, Dong-Ya</creator><creator>Wang, Jin</creator><creator>Li, Xiao-Bo</creator><creator>Song, Xin-Ying</creator><creator>Yuan, Yong</creator><creator>Fan, Xi-Long</creator><creator>Zhao, Xiao-Yun</creator><creator>Huang, Yue</creator><creator>Ma, Xiang</creator><creator>Zhang, Peng</creator><creator>Li, Bing</creator><creator>Ge, Ming-Yu</creator><creator>Tuo, You-Li</creator><creator>Chen, Wei</creator><creator>Zhang, Hong-Mei</creator><creator>He, Jian-Jian</creator><creator>Li, Chao-Yang</creator><creator>Yi, Qi-Bin</creator><creator>Zhao, Yi</creator><creator>Zhang, Yan-Qiu</creator><creator>Zheng, Chao</creator><creator>Xue, Wang-Chen</creator><creator>Liu, Jia-Cong</creator><creator>Zhang, Zhen</creator><creator>Li, Cheng-Kui</creator><creator>Zhang, Xiao-Lu</creator><creator>Zhao, Hong-Yu</creator><creator>Zhao, Guo-Ying</creator><creator>Guo, Zhi-Wei</creator><creator>Xie, Sheng-Lun</creator><creator>Wang, Chen-Wei</creator><creator>Zhang, Bo-Xin</creator><creator>Wang, Yue</creator><creator>Li, Qing-Xin</creator><creator>Li, Chao</creator><creator>Zhang, Kai</creator><creator>Shi, Dong-Li</creator><creator>Zhao, Shi-Yi</creator><creator>Yao, Min</creator><creator>An, Zheng-Hua</creator><creator>Chen, Chan</creator><creator>Gong, Ke</creator><creator>Liu, Ya-Qing</creator><creator>Gao, Min</creator><creator>Li, Xin-Qiao</creator><creator>Li, Yan-Guo</creator><creator>Liang, Xiao-Hua</creator><creator>Liu, Xiao-Jing</creator><creator>Sun, Xi-Lei</creator><creator>Wang, Jin-Zhou</creator><creator>Wen, Xiang-Yang</creator><creator>Xu, Yan-Bing</creator><creator>Xu, Yu-Peng</creator><creator>Yang, Sheng</creator><creator>Zhang, Chao-Yue</creator><creator>Zhang, Da-Li</creator><creator>Zhang, Fei</creator><creator>Chen, Gang</creator><creator>Lu, Fang-Jun</creator><creator>Sun, Gong-Xing</creator><creator>Zhang, Fan</creator><creator>Zhang, Shuang-Nan</creator><general>Oxford University Press</general><scope>TOX</scope><scope>AAYXX</scope><scope>CITATION</scope><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></search><sort><creationdate>20220617</creationdate><title>Energetic transients joint analysis system for multi-INstrument (ETJASMIN) for GECAM – I. 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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> |
fulltext | fulltext |
identifier | ISSN: 0035-8711 |
ispartof | Monthly notices of the Royal Astronomical Society, 2022-06, Vol.514 (2), p.2397-2406 |
issn | 0035-8711 1365-2966 |
language | eng |
recordid | cdi_crossref_primary_10_1093_mnras_stac999 |
source | Oxford Journals Open Access Collection |
title | Energetic transients joint analysis system for multi-INstrument (ETJASMIN) for GECAM – I. Positional, temporal, and spectral analyses |
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