The First Insight-HXMT Localization Catalog of Short-duration Gamma-Ray Bursts: The First Six Years
As of 2023 December, the high-energy telescope (HE) of Insight-HXMT has detected 72 short-duration gamma-ray bursts (sGRBs), which may be related to binary compact star mergers. In this work, we locate these sGRBs by adopting an enhanced time-delay localization method based on the Li modified cross-...
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| author | Shuo Xiao Yan-Ting Zhang Yue Wang Yan-Qiu Zhang Shao-Lin Xiong Shuang-Nan Zhang Shi-Jie Zheng Jin-Peng Zhang Peng Zhang Cheng-Kui Li Xiao-Bo Li Shu-Xu Yi Zhen Zhang Bing Li Hua Feng Cong-Zhan Liu Ming-Yu Ge Xu-Fang Li Zheng-Wei Li Yu-Peng Xu Xiang-Yang Wen Jian-Chao Sun Lian Tao Qi-Bin Yi Ce Cai Yi Zhao Wang-Chen Xue Jia-Cong Liu Chao Zheng Chen-Wei Wang Wen-Jun Tan You-Li Tuo Li-Ming Song Fang-Jun Lu Ti-Pei Li |
| author_facet | Shuo Xiao Yan-Ting Zhang Yue Wang Yan-Qiu Zhang Shao-Lin Xiong Shuang-Nan Zhang Shi-Jie Zheng Jin-Peng Zhang Peng Zhang Cheng-Kui Li Xiao-Bo Li Shu-Xu Yi Zhen Zhang Bing Li Hua Feng Cong-Zhan Liu Ming-Yu Ge Xu-Fang Li Zheng-Wei Li Yu-Peng Xu Xiang-Yang Wen Jian-Chao Sun Lian Tao Qi-Bin Yi Ce Cai Yi Zhao Wang-Chen Xue Jia-Cong Liu Chao Zheng Chen-Wei Wang Wen-Jun Tan You-Li Tuo Li-Ming Song Fang-Jun Lu Ti-Pei Li |
| author_sort | Shuo Xiao |
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| description | As of 2023 December, the high-energy telescope (HE) of Insight-HXMT has detected 72 short-duration gamma-ray bursts (sGRBs), which may be related to binary compact star mergers. In this work, we locate these sGRBs by adopting an enhanced time-delay localization method based on the Li modified cross-correlation function (Li-CCF), jointly with Insight-HXMT/HE, Gravitational-wave high-energy Electromagnetic Counterpart All-sky Monitor, Fermi/Gamma-ray Burst Monitor (GBM), INTEGRAL/SPI-ACS, and Konus-Wind. The results indicate that joint localization improves accuracy (3 σ ) by an average of 59% compared to results with GBM alone, and the participation of HXMT improves the joint localization accuracy (3 σ ) by an average of 47%. The median and minimum of the joint localization area are 229 and 0.2 square degrees, respectively. We also propose a method to effectively locate those bursts (e.g., GRB 200415A) for which HE suffered from data saturation. In addition, we investigate whether the multiple annuli are independent when there is overlapping data through simulations. The results show that as long as the data from both satellites used have not been overlapped at the same time, the localization results (annuli) are independent. Finally, we verify the robustness of the results by comparing the precise localization bursts observed by Swift/Burst Alert Telescope, as well as publishing the high-time-resolution light curves, orbits and localization probability sky maps in Hierarchical Equal Area Isolatitude Pixelization format files on the website https://ihepbox.ihep.ac.cn/ihepbox/index.php/s/LO1eRZ0SBIEiBIg . |
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| spelling | doaj-art-69af9929fbfa48cd85fe4098a76f32742025-08-20T02:35:46ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492025-01-0127826010.3847/1538-4365/add5eeThe First Insight-HXMT Localization Catalog of Short-duration Gamma-Ray Bursts: The First Six YearsShuo Xiao0https://orcid.org/0000-0003-2957-2806Yan-Ting Zhang1Yue Wang2https://orcid.org/0009-0008-5068-3504Yan-Qiu Zhang3Shao-Lin Xiong4https://orcid.org/0000-0002-4771-7653Shuang-Nan Zhang5https://orcid.org/0000-0001-5586-1017Shi-Jie Zheng6Jin-Peng Zhang7Peng Zhang8https://orcid.org/0000-0002-8097-3616Cheng-Kui Li9https://orcid.org/0000-0001-5798-4491Xiao-Bo Li10https://orcid.org/0000-0003-4585-589XShu-Xu Yi11https://orcid.org/0000-0001-7599-0174Zhen Zhang12https://orcid.org/0000-0003-4673-773XBing Li13https://orcid.org/0000-0002-0238-834XHua Feng14https://orcid.org/0000-0001-7584-6236Cong-Zhan Liu15Ming-Yu Ge16https://orcid.org/0000-0002-2749-6638Xu-Fang Li17https://orcid.org/0000-0002-2793-9857Zheng-Wei Li18Yu-Peng Xu19https://orcid.org/0000-0002-8476-9217Xiang-Yang Wen20Jian-Chao Sun21Lian Tao22https://orcid.org/0000-0002-2705-4338Qi-Bin Yi23Ce Cai24https://orcid.org/0000-0002-6540-2372Yi Zhao25Wang-Chen Xue26https://orcid.org/0000-0001-8664-5085Jia-Cong Liu27Chao Zheng28Chen-Wei Wang29https://orcid.org/0009-0008-8053-2985Wen-Jun Tan30You-Li Tuo31https://orcid.org/0000-0003-3127-0110Li-Ming Song32https://orcid.org/0000-0003-0274-3396Fang-Jun Lu33https://orcid.org/0000-0003-3248-6087Ti-Pei Li34School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiaoshuo@gznu.edu.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; College of Electronic and Information Engineering, Tongji University , Shanghai 201804, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; Key Laboratory of Stellar and Interstellar Physics and Department of Physics, Xiangtan University , 411105 Xiangtan, Hunan Province, People’s Republic of ChinaCollege of Physics, Hebei Normal University , 20 South Erhuan Road, Shijiazhuang, 050024, People’s Republic of ChinaSchool of Computer and Information, Dezhou University , Dezhou 253023, Shandong, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of ChinaInstitut für Astronomie und Astrophysik , University of Tübingen, Sand 1, 72076 Tübingen, GermanyKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of ChinaKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cnKey Laboratory of Particle Astrophysics , Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China ; xiongsl@ihep.ac.cn, zhangsn@ihep.ac.cn; Department of Astronomy, Tsinghua University , Beijing 100084, People’s Republic of ChinaAs of 2023 December, the high-energy telescope (HE) of Insight-HXMT has detected 72 short-duration gamma-ray bursts (sGRBs), which may be related to binary compact star mergers. In this work, we locate these sGRBs by adopting an enhanced time-delay localization method based on the Li modified cross-correlation function (Li-CCF), jointly with Insight-HXMT/HE, Gravitational-wave high-energy Electromagnetic Counterpart All-sky Monitor, Fermi/Gamma-ray Burst Monitor (GBM), INTEGRAL/SPI-ACS, and Konus-Wind. The results indicate that joint localization improves accuracy (3 σ ) by an average of 59% compared to results with GBM alone, and the participation of HXMT improves the joint localization accuracy (3 σ ) by an average of 47%. The median and minimum of the joint localization area are 229 and 0.2 square degrees, respectively. We also propose a method to effectively locate those bursts (e.g., GRB 200415A) for which HE suffered from data saturation. In addition, we investigate whether the multiple annuli are independent when there is overlapping data through simulations. The results show that as long as the data from both satellites used have not been overlapped at the same time, the localization results (annuli) are independent. Finally, we verify the robustness of the results by comparing the precise localization bursts observed by Swift/Burst Alert Telescope, as well as publishing the high-time-resolution light curves, orbits and localization probability sky maps in Hierarchical Equal Area Isolatitude Pixelization format files on the website https://ihepbox.ihep.ac.cn/ihepbox/index.php/s/LO1eRZ0SBIEiBIg .https://doi.org/10.3847/1538-4365/add5eeGamma-ray bursts |
| spellingShingle | Shuo Xiao Yan-Ting Zhang Yue Wang Yan-Qiu Zhang Shao-Lin Xiong Shuang-Nan Zhang Shi-Jie Zheng Jin-Peng Zhang Peng Zhang Cheng-Kui Li Xiao-Bo Li Shu-Xu Yi Zhen Zhang Bing Li Hua Feng Cong-Zhan Liu Ming-Yu Ge Xu-Fang Li Zheng-Wei Li Yu-Peng Xu Xiang-Yang Wen Jian-Chao Sun Lian Tao Qi-Bin Yi Ce Cai Yi Zhao Wang-Chen Xue Jia-Cong Liu Chao Zheng Chen-Wei Wang Wen-Jun Tan You-Li Tuo Li-Ming Song Fang-Jun Lu Ti-Pei Li The First Insight-HXMT Localization Catalog of Short-duration Gamma-Ray Bursts: The First Six Years The Astrophysical Journal Supplement Series Gamma-ray bursts |
| title | The First Insight-HXMT Localization Catalog of Short-duration Gamma-Ray Bursts: The First Six Years |
| title_full | The First Insight-HXMT Localization Catalog of Short-duration Gamma-Ray Bursts: The First Six Years |
| title_fullStr | The First Insight-HXMT Localization Catalog of Short-duration Gamma-Ray Bursts: The First Six Years |
| title_full_unstemmed | The First Insight-HXMT Localization Catalog of Short-duration Gamma-Ray Bursts: The First Six Years |
| title_short | The First Insight-HXMT Localization Catalog of Short-duration Gamma-Ray Bursts: The First Six Years |
| title_sort | first insight hxmt localization catalog of short duration gamma ray bursts the first six years |
| topic | Gamma-ray bursts |
| url | https://doi.org/10.3847/1538-4365/add5ee |
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