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相关论文: EP240801a/XRF 240801B: An X-ray Flash Detected by …

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X-ray flashes (XRFs) are fast X-ray transients thought to be softer analogs of gamma-ray bursts (GRBs). With its soft X-ray sensitivity, the Einstein Probe (EP) provides a unique opportunity to study these events. We report multiwavelength…

We present multi-wavelength study of the $\gamma$/X-ray transient EP250416a (also designated GRB 250416C), triggered by the Einstein Probe (EP) Wide-field X-ray Telescope and also by SVOM and Konus-Wind. Observations spanning the gamma-ray,…

Fast X-ray Transients (FXTs) represent a new class of highly luminous transients in soft X-rays ($\sim$0.3-10 keV) associated with violent astrophysical processes. They manifest as short, singular flashes of X-ray photons with durations…

The Einstein Probe (EP) satellite, dedicated at time-domain high-energy astrophysics and multi-messenger astronomy, was recently launched and successfully put into operation. The wide-field X-ray telescope (WXT, 0.5-4 keV) onboard has…

高能天体物理现象 · 物理学 2025-04-22 Hao-Xuan Gao , Jin-Jun Geng , Yi-Fang Liang , Hui Sun , Fan Xu , Xue-Feng Wu , Yong-Feng Huang , Zi-Gao Dai , Wei-Min Yuan

Long gamma-ray bursts (LGRBs), including their subclasses of low-luminosity GRBs (LL-GRBs) and X-ray flashes (XRFs) characterized by low spectral peak energies, are known to be associated with broad-lined Type Ic supernovae (SNe Ic-BL),…

EP241217a is an X-ray transient detected by the Einstein Probe (EP) lasting for about 100 seconds and without accompanying $\gamma$-ray detection. The optical spectroscopy reveals the redshift of EP241217a is 4.59. By combining the…

Long gamma-ray bursts (GRBs) are believed to originate from core collapse of massive stars. High-redshift GRBs can probe the star formation and reionization history of the early universe, but their detection remains rare. Here we report the…

高能天体物理现象 · 物理学 2024-04-26 Y. Liu , H. Sun , D. Xu , D. S. Svinkin , J. Delaunay , N. R. Tanvir , H. Gao , C. Zhang , Y. Chen , X. -F. Wu , B. Zhang , W. Yuan , J. An , G. Bruni , D. D. Frederiks , G. Ghirlanda , J. -W. Hu , A. Li , C. -K. Li , J. -D. Li , D. B. Malesani , L. Piro , G. Raman , R. Ricci , E. Troja , S. D. Vergani , Q. -Y. Wu , J. Yang , B. -B. Zhang , Z. -P. Zhu , A. de Ugarte Postigo , A. G. Demin , D. Dobie , Z. Fan , S. -Y. Fu , J. P. U. Fynbo , J. -J. Geng , G. Gianfagna , Y. -D. Hu , Y. -F. Huang , S. -Q. Jiang , P. G. Jonker , Y. Julakanti , J. A. Kennea , A. A. Kokomov , E. Kuulkers , W. -H. Lei , J. K. Leung , A. J. Levan , D. -Y. Li , Y. Li , S. P. Littlefair , X. Liu , A. L. Lysenko , Y. -N. Ma , A. Martin-Carrillo , P. O'Brien , T. Parsotan , J. Quirola-Vasquez , A. V. Ridnaia , S. Ronchini , A. Rossi , D. Mata-Sanchez , B. Schneider , R. -F. Shen , A. L. Thakur , A. Tohuvavohu , M. A. P. Torres , A. E. Tsvetkova , M. V. Ulanov , J. -J. Wei , D. Xiao , Y. -H. I. Yin , M. Bai , V. Burwitz , Z. -M. Cai , F. -S. Chen , H. -L. Chen , T. -X. Chen , W. Chen , Y. -F. Chen , Y. -H. Chen , H. -Q. Cheng , C. -Z. Cui , W. -W. Cui , Y. -F. Dai , Z. -G. Dai , J. Eder , D. -W. Fan , C. Feldman , H. Feng , Z. Feng , P. Friedrich , X. Gao , J. Guan , D. -W Han , J. Han , D. -J. Hou , H. -B. Hu , T. Hu , M. -H. Huang , J. Huo , I. Hutchinson , Z. Ji , S. -M. Jia , Z. -Q. Jia , B. -W. Jiang , C. -C. Jin , G. Jin , J. -J. Jin , A. Keereman , H. Lerman , J. -F. Li , L. -H. Li , M. -S. Li , W. Li , Z. -D. Li , T. -Y. Lian , E. -W. Liang , Z. -X. Ling , C. -Z. Liu , H. -Y. Liu , H. -Q. Liu , M. -J. Liu , Y. -R. Liu , F. -J. Lu , H. -J. LU , L. -D. Luo , F. L. Ma , J. Ma , J. -R. Mao , X. Mao , M. McHugh , N. Meidinger , K. Nandra , J. P. Osborne , H. -W. Pan , X. Pan , M. E. Ravasio , A. Rau , N. Rea , U. Rehman , J. Sanders , A. Santovincenzo , L. -M. Song , J. Su , L. -J. Sun , S. -L. Sun , X. -J. Sun , Y. -Y. Tan , Q. -J. Tang , Y. -H. Tao , J. -Z. Tong , H. Wang , J. Wang , L. Wang , W. -X. Wang , X. -F. Wang , X. -Y. Wang , Y. -L. Wang , Y. -S. Wang , D. -M. Wei , R. Willingale , S. -L. Xiong , H. -T. Xu , J. -J. Xu , X. -P. Xu , Y. -F. Xu , Z. Xu , C. -B. Xue , Y. -L. Xue , A. -L. Yan , F. Yang , H. -N. Yang , X. -T. Yang , Y. -J Yang , Y. -W. Yu , J. Zhang , M. Zhang , S. -N. Zhang , W. -D. Zhang , W. -J. Zhang , Y. -H. Zhang , Z. Zhang , Z. Zhang , Z. -L. Zhang , D. -H. Zhao , H. -S. Zhao , X. -F. Zhao , Z. -J. Zhao , L. -X. Zhou , Y. -L. Zhou , Y. -X. Zhu , Z. -C. Zhu , X. -X. Zuo

We present the results of our multi-wavelength (X-ray to radio) follow-up campaign of the Einstein Probe transient EP240408a. The initial 10 s trigger displayed bright soft X-ray (0.5-4 keV) radiation with peak luminosity $L_\textrm{X}…

The recent Einstein Probe (EP) event EP240414a exhibits several unusual observational features. Its prompt and afterglow emissions place it between long gamma-ray bursts (LGRBs) and low-luminosity GRBs (LLGRBs). The event is followed by a…

高能天体物理现象 · 物理学 2025-05-27 Hamid Hamidani , Yuri Sato , Kazumi Kashiyama , Masaomi Tanaka , Kunihito Ioka , Shigeo S. Kimura

Despite being operational for only a short time, the Einstein Probe mission, with its large field of view and rapid localisation capabilities, has already significantly advanced the study of rapid variability in the soft X-ray sky. We…

The recent launch of Einstein Probe (EP) in early 2024 opened up a new window onto the transient X-ray sky, allowing for real-time discovery and follow-up of fast X-ray transients (FXRTs). Multi-wavelength observations of FXRTs and their…

高能天体物理现象 · 物理学 2024-07-29 R. Ricci , E. Troja , Y. Yang , M. Yadav , Y. Liu , H. Sun , X. Wu , H. Gao , B. Zhang , W. Yuan

We present a multi-wavelength analysis of the fast X-ray transient EP 241021a, discovered by the Wide-field X-ray Telescope aboard the \emph{Einstein Probe} satellite on 2024 October 21. The event was not detected in gamma-rays. Follow-up…

We report the discovery of a peculiar X-ray transient, EP240408a, by Einstein Probe (EP) and follow-up studies made with EP, Swift, NICER, GROND, ATCA and other ground-based multi-wavelength telescopes. The new transient was first detected…

高能天体物理现象 · 物理学 2024-10-30 Wenda Zhang , Weimin Yuan , Zhixing Ling , Yong Chen , Nanda Rea , Arne Rau , Zhiming Cai , Huaqing Cheng , Francesco Coti Zelati , Lixin Dai , Jingwei Hu , Shumei Jia , Chichuan Jin , Dongyue Li , Paul O'Brien , Rongfeng Shen , Xinwen Shu , Shengli Sun , Xiaojin Sun , Xiaofeng Wang , Lei Yang , Bing Zhang , Chen Zhang , Shuang-Nan Zhang , Yonghe Zhang , Jie An , David Buckley , Alexis Coleiro , Bertrand Cordier , Liming Dou , Rob Eyles-Ferris , Zhou Fan , Hua Feng , Shaoyu Fu , Johan P. U. Fynbo , Lluis Galbany , Saurabh W. Jha , Shuaiqing Jiang , Albert Kong , Erik Kuulkers , Weihua Lei , Wenxiong Li , Bifang Liu , Mingjun Liu , Xing Liu , Yuan Liu , Zhu Liu , Chandreyee Maitra , Alessio Marino , Itumeleng Monageng , Kirpal Nandra , Jeremy Sanders , Roberto Soria , Lian Tao , Junfeng Wang , Song Wang , Tinggui Wang , Zhongxiang Wang , Qingwen Wu , Xuefeng Wu , Dong Xu , Yanjun Xu , Suijian Xue , Yongquan Xue , Zijian Zhang , Zipei Zhu , Hu Zou , Congying Bao , Fansheng Chen , Houlei Chen , Tianxiang Chen , Wei Chen , Yehai Chen , Yifan Chen , Chenzhou Cui , Weiwei Cui , Yanfeng Dai , Dongwei Fan , Ju Guan , Dawei Han , Dongjie Hou , Haibo Hu , Maohai Huang , Jia Huo , Zhenqing Jia , Bowen Jiang , Ge Jin , Chengkui Li , Junfei Li , Longhui Li , Maoshun Li , Wei Li , Zhengda Li , Tianying Lian , Congzhan Liu , Heyang Liu , Huaqiu Liu , Fangjun Lu , Laidan Luo , Jia Ma , Xuan Mao , Haiwu Pan , Xin Pan , Liming Song , Hui Sun , Yunyin Tan , Qingjun Tang , Yihan Tao , Hao Wang , Juan Wang , Lei Wang , Wenxin Wang , Yilong Wang , Yusa Wang , Qinyu Wu , Haitao Xu , Jingjing Xu , Xinpeng Xu , Yunfei Xu , Zhao Xu , Changbin Xue , Yulong Xue , Ailiang Yan , Haonan Yang , Xiongtao Yang , Yanji Yang , Juan Zhang , Mo Zhang , Wenjie Zhang , Zhen Zhang , Zhen Zhang , Ziliang Zhang , Donghua Zhao , Haisheng Zhao , Xiaofan Zhao , Zijian Zhao , Hongyan Zhou , Yilin Zhou , Yuxuan Zhu , Zhencai Zhu

Fast X-ray transients (FXRTs) are short-lived X-ray outbursts with diverse progenitor scenarios, including compact object mergers, stellar core-collapses and tidal disruption events. The Einstein Probe (EP) has enabled the rapid discovery…

We present James Webb Space Telescope (JWST) and Hubble Space Telescope (HST) observations of the counterpart of EP240801a, at z=1.67, the first fast X-ray transient (FXT) identified as an X-ray flash (XRF) by the Einstein Probe (EP) and…

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