_version_ 1866914476993806336
author Fu, Shao-Yu
Dai, Cui-Yuan
Wang, Ai-Ling
Xu, Dong
An, Tao
Geng, Jin-Jun
Lei, Wei-Hua
Wang, Xiang-Yu
Jiang, Shuai-Qing
Zhu, Zi-Pei
Liu, Xing
An, Jie
He, Lin-Bo
Jin, Jun-Jie
Zhang, Yu
Zhang, Jinlei
Fan, Zhou
Gao, Xing
Iskandar, Abdusamatjan
Yaqup, Shahidin
Zhong, Tu-Hong
Esamdin, Ali
Bai, Chun-Hai
Zhang, Yu
Gao, He
Wu, Xue-Feng
Malesani, Daniele Bjørn
Izzo, Luca
Eyles-Ferris, R. A. J.
Saccardi, A.
Schneider, B.
Palmerio, J.
Tanvir, N. R.
Pozanenko, Alexei
Pankov, Nicolai
Moskvitin, A. S.
Spiridonova, O. I.
Maslennikova, O. A.
Volnova, A.
Klunko, E.
Rumyantsev, V.
Volvach, A.
Volvach, L.
Komesh, Toktarkhan
Abdikamalov, Ernazar
Berdikhan, Dilda
Maksut, Zhanat
Zou, Yuan-Chuan
Wu, Hong-Zhou
Yu, Yun-Wei
Shen, Rong-Feng
Wang, Yi-Han
Sun, Hui
Zhang, Bin-Bin
Liu, Liang-Duan
Li, Ye
D'Elia, Valerio
Salvaterra, Ruben
De Pasquale, Massimiliano
Zhang, Bing
Yuan, Wei-Min
author_facet Fu, Shao-Yu
Dai, Cui-Yuan
Wang, Ai-Ling
Xu, Dong
An, Tao
Geng, Jin-Jun
Lei, Wei-Hua
Wang, Xiang-Yu
Jiang, Shuai-Qing
Zhu, Zi-Pei
Liu, Xing
An, Jie
He, Lin-Bo
Jin, Jun-Jie
Zhang, Yu
Zhang, Jinlei
Fan, Zhou
Gao, Xing
Iskandar, Abdusamatjan
Yaqup, Shahidin
Zhong, Tu-Hong
Esamdin, Ali
Bai, Chun-Hai
Zhang, Yu
Gao, He
Wu, Xue-Feng
Malesani, Daniele Bjørn
Izzo, Luca
Eyles-Ferris, R. A. J.
Saccardi, A.
Schneider, B.
Palmerio, J.
Tanvir, N. R.
Pozanenko, Alexei
Pankov, Nicolai
Moskvitin, A. S.
Spiridonova, O. I.
Maslennikova, O. A.
Volnova, A.
Klunko, E.
Rumyantsev, V.
Volvach, A.
Volvach, L.
Komesh, Toktarkhan
Abdikamalov, Ernazar
Berdikhan, Dilda
Maksut, Zhanat
Zou, Yuan-Chuan
Wu, Hong-Zhou
Yu, Yun-Wei
Shen, Rong-Feng
Wang, Yi-Han
Sun, Hui
Zhang, Bin-Bin
Liu, Liang-Duan
Li, Ye
D'Elia, Valerio
Salvaterra, Ruben
De Pasquale, Massimiliano
Zhang, Bing
Yuan, Wei-Min
contents Extragalactic Fast X-ray Transients (EFXTs) represent an emerging class of high-energy phenomena characterized by X-ray outbursts lasting from tens to hundreds of seconds. However, for more than half of the EFXTs, their physical origins remain elusive. In this Letter, we report the discovery of EP250302a, a luminous EFXT detected by the Einstein Probe (EP) at a redshift of $z = 1.131$. The multi-wavelength light curves of EP250302a reveal remarkable temporal features that distinguish it from the previously known EP-detected EFXT population, most notably a needle-like X-ray flare accompanied by smooth optical rebrightening during the afterglow phase. We suggest that the distinct X-ray and optical behaviors constitute the first observed instance of late-time violent collision of two relativistic shells in an EFXT. Drawing on insights from GRB studies, such a collision process strongly indicates the reactivation of a central engine, making EP250302a-like transients a unique laboratory for probing the late-time activity and jet physics of EFXT central engines.
format Preprint
id arxiv_https___arxiv_org_abs_2604_14341
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle A fast X-ray transient with chromatic flares: signatures of violent collisions induced by late-time central engine reactivation
Fu, Shao-Yu
Dai, Cui-Yuan
Wang, Ai-Ling
Xu, Dong
An, Tao
Geng, Jin-Jun
Lei, Wei-Hua
Wang, Xiang-Yu
Jiang, Shuai-Qing
Zhu, Zi-Pei
Liu, Xing
An, Jie
He, Lin-Bo
Jin, Jun-Jie
Zhang, Yu
Zhang, Jinlei
Fan, Zhou
Gao, Xing
Iskandar, Abdusamatjan
Yaqup, Shahidin
Zhong, Tu-Hong
Esamdin, Ali
Bai, Chun-Hai
Zhang, Yu
Gao, He
Wu, Xue-Feng
Malesani, Daniele Bjørn
Izzo, Luca
Eyles-Ferris, R. A. J.
Saccardi, A.
Schneider, B.
Palmerio, J.
Tanvir, N. R.
Pozanenko, Alexei
Pankov, Nicolai
Moskvitin, A. S.
Spiridonova, O. I.
Maslennikova, O. A.
Volnova, A.
Klunko, E.
Rumyantsev, V.
Volvach, A.
Volvach, L.
Komesh, Toktarkhan
Abdikamalov, Ernazar
Berdikhan, Dilda
Maksut, Zhanat
Zou, Yuan-Chuan
Wu, Hong-Zhou
Yu, Yun-Wei
Shen, Rong-Feng
Wang, Yi-Han
Sun, Hui
Zhang, Bin-Bin
Liu, Liang-Duan
Li, Ye
D'Elia, Valerio
Salvaterra, Ruben
De Pasquale, Massimiliano
Zhang, Bing
Yuan, Wei-Min
High Energy Astrophysical Phenomena
Extragalactic Fast X-ray Transients (EFXTs) represent an emerging class of high-energy phenomena characterized by X-ray outbursts lasting from tens to hundreds of seconds. However, for more than half of the EFXTs, their physical origins remain elusive. In this Letter, we report the discovery of EP250302a, a luminous EFXT detected by the Einstein Probe (EP) at a redshift of $z = 1.131$. The multi-wavelength light curves of EP250302a reveal remarkable temporal features that distinguish it from the previously known EP-detected EFXT population, most notably a needle-like X-ray flare accompanied by smooth optical rebrightening during the afterglow phase. We suggest that the distinct X-ray and optical behaviors constitute the first observed instance of late-time violent collision of two relativistic shells in an EFXT. Drawing on insights from GRB studies, such a collision process strongly indicates the reactivation of a central engine, making EP250302a-like transients a unique laboratory for probing the late-time activity and jet physics of EFXT central engines.
title A fast X-ray transient with chromatic flares: signatures of violent collisions induced by late-time central engine reactivation
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2604.14341