Multi-instrument Search for Gamma-Ray Counterpart of X-Ray Transients Detected by EP/WXT
As a soft X-ray imager with an unprecedentedly large field of view, Einstein Probe (EP)/Wide-field X-ray Telescope (WXT) has detected many (fast) X-ray transients, whose nature is very intriguing. Whether there is a gamma-ray counterpart for the X-ray transient provides important implications for it...
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Published in | Astrophysical journal. Letters Vol. 987; no. 2; p. L38 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
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The American Astronomical Society
10.07.2025
IOP Publishing |
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Abstract | As a soft X-ray imager with an unprecedentedly large field of view, Einstein Probe (EP)/Wide-field X-ray Telescope (WXT) has detected many (fast) X-ray transients, whose nature is very intriguing. Whether there is a gamma-ray counterpart for the X-ray transient provides important implications for its origin. Some of them have been reported to be associated with gamma-ray bursts; however, a systematic study on the gamma-ray emission of these X-ray transients is lacking. In this work, we implemented a comprehensive targeted search for gamma-ray counterparts to 63 X-ray transients reported by EP/WXT during its first year of operation, using the dedicated multiple-instrument search pipeline, Energetic Transients Joint Analysis System for Multi-Instrument (ETJASMIN), with GECAM-B, GECAM-C, Fermi/GBM, and Insight-HXMT data. We find that 14 out of 63 (22%) EP/WXT X-ray transients have gamma-ray counterparts. For other transients, the ETJASMIN pipeline provided the upper limit of the gamma-ray emission, which is more stringent than that given by an individual instrument. Moreover, we investigated the properties of the X-ray transients and their gamma-ray counterparts and explored the relation between the X-ray transient and the gamma-ray counterpart. |
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AbstractList | As a soft X-ray imager with an unprecedentedly large field of view, Einstein Probe (EP)/Wide-field X-ray Telescope (WXT) has detected many (fast) X-ray transients, whose nature is very intriguing. Whether there is a gamma-ray counterpart for the X-ray transient provides important implications for its origin. Some of them have been reported to be associated with gamma-ray bursts; however, a systematic study on the gamma-ray emission of these X-ray transients is lacking. In this work, we implemented a comprehensive targeted search for gamma-ray counterparts to 63 X-ray transients reported by EP/WXT during its first year of operation, using the dedicated multiple-instrument search pipeline, Energetic Transients Joint Analysis System for Multi-Instrument (ETJASMIN), with GECAM-B, GECAM-C, Fermi/GBM, and Insight-HXMT data. We find that 14 out of 63 (22%) EP/WXT X-ray transients have gamma-ray counterparts. For other transients, the ETJASMIN pipeline provided the upper limit of the gamma-ray emission, which is more stringent than that given by an individual instrument. Moreover, we investigated the properties of the X-ray transients and their gamma-ray counterparts and explored the relation between the X-ray transient and the gamma-ray counterpart. |
Author | Yu, Zheng-Hang Cai, Ce Zhang, Peng Li, Xiao-Bo Zhang, Yan-Qiu Xiong, Shao-Lin Wang, Chen-Wei Zhang, Wen-Long Zhang, Shuang-Nan Zheng, Shi-Jie Zheng, Chao Tan, Wen-Jun Huang, Yue Ren, Yang-Zhao Liu, Jia-Cong Zhang, Zhen Yi, Shu-Xu Guo, Hao-Xuan Xue, Wang-Chen Wang, Ping Zhang, Jin-Peng Liu, Yuan Wang, Yue Zhao, Xiao-Yun Li, Cheng-Kui Xiao, Shuo Xie, Sheng-Lun Song, Li-Ming |
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University of Chinese Academy of Sciences , Chinese Academy of Sciences, Beijing 100049, People’s Republic of China – sequence: 19 givenname: Yang-Zhao surname: Ren fullname: Ren, Yang-Zhao organization: Southwest Jiaotong University School of Physical Science and Technology, Chengdu 611756, Sichuan, People’s Republic of China – sequence: 20 givenname: Ping orcidid: 0000-0003-0466-2223 surname: Wang fullname: Wang, Ping organization: Chinese Academy of Sciences State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Beijing 100049, xiongsl@ihep.ac.cn People’s Republic of China – sequence: 21 givenname: Yue surname: Huang fullname: Huang, Yue organization: Chinese Academy of Sciences State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Beijing 100049, xiongsl@ihep.ac.cn People’s Republic of China – sequence: 22 givenname: Xiao-Bo surname: Li fullname: Li, Xiao-Bo organization: Chinese Academy of Sciences State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Beijing 100049, xiongsl@ihep.ac.cn People’s Republic of China – sequence: 23 givenname: Xiao-Yun surname: Zhao fullname: Zhao, Xiao-Yun organization: Chinese Academy of Sciences State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Beijing 100049, xiongsl@ihep.ac.cn People’s Republic of China – sequence: 24 givenname: Shi-Jie surname: Zheng fullname: Zheng, Shi-Jie organization: Chinese Academy of Sciences State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Beijing 100049, xiongsl@ihep.ac.cn People’s Republic of China – sequence: 25 givenname: Zhen orcidid: 0000-0003-4673-773X surname: Zhang fullname: Zhang, Zhen organization: Chinese Academy of Sciences State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Beijing 100049, xiongsl@ihep.ac.cn People’s Republic of China – sequence: 26 givenname: Shu-Xu surname: Yi fullname: Yi, Shu-Xu organization: Chinese Academy of Sciences State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Beijing 100049, xiongsl@ihep.ac.cn People’s Republic of China – sequence: 27 givenname: Li-Ming orcidid: 0000-0003-0274-3396 surname: Song fullname: Song, Li-Ming organization: Chinese Academy of Sciences State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Beijing 100049, xiongsl@ihep.ac.cn People’s Republic of China – sequence: 28 givenname: Shuang-Nan orcidid: 0000-0001-5586-1017 surname: Zhang fullname: Zhang, Shuang-Nan organization: Chinese Academy of Sciences State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Beijing 100049, xiongsl@ihep.ac.cn People’s Republic of China |
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SubjectTerms | Gamma-ray bursts Gamma-ray observatories X-ray transient sources |
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Title | Multi-instrument Search for Gamma-Ray Counterpart of X-Ray Transients Detected by EP/WXT |
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