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Main Authors: Li, An, Wang, Chen-Wei, Passaleva, Niccolò, An, Jie, Zhang, Bin-Bin, Troja, Eleonora, Yin, Yi-Han Iris, Liu, Yuan, Xiong, Shao-Lin, Xin, Li-Ping, Shao, Yi-Xuan, Yang, Jun, Sun, Hui, Xu, Dong, Yang, Yu-Han, Ricci, Roberto, Gao, He, Antier, Sarah, Becerra, Rosa L., Cao, Jia-Xin, Castro-Tirado, Alberto Javier, Chen, Xin-Lei, Cheng, Ye-Hao, Chen, Yong, Cheng, Hua-Qing, D'Elia, Valerio, De Pasquale, Massimiliano, Dong, Yong-Wei, Elhosseiny, Eslam, Eyles-Ferris, Rob A. J., Gritsevich, Maria, Han, Xu-Hui, Hartmann, Dieter, Hu, You-Dong, Hu, Jing-Wei, Jia, Shu-Mei, Kochiashvili, Nino, Lei, Wei-Hua, Levan, Andrew J., Li, Cheng-Kui, Li, Dong-Yue, Li, Hua-Li, Li, Xiao-Bo, Ling, Zhi-Xing, Liu, He-Yang, Lv, Hou-Jun, Malesani, Daniele B., O'Connor, Brendan, Pan, Hai-Wu, Pandey, Shashi Bhushan, Perez-Garcia, Ignacio, Pieterse, Daniëlle L. A., Pillas, Marion, Qiu, Yu-Lei, Saccardi, Andrea, Sánchez-Ramírez, Rubén, Tan, Wen-Jun, Tanasan, Manasanun, Tanvir, Nial R., Vergani, Susanna D., Wang, Jing, Wang, Xiao-Feng, Wu, Qin-Yu, Yi, Shu-Xu, Yusufjon, Tillayev, Zhang, Chen, Zhang, Wen-Da, Zhang, Yi-Jia, Zhao, Guo-Ying, Zheng, Chao, Zheng, Shi-Jie, Zhou, Chang, Zhou, Ping, Cordier, Bertrand, Wei, Jian-Yan, Yuan, Weimin, Zhang, Shuang-Nan, Zhang, Bing
Format: Preprint
Published: 2026
Subjects:
Online Access:https://arxiv.org/abs/2601.14137
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author Li, An
Wang, Chen-Wei
Passaleva, Niccolò
An, Jie
Zhang, Bin-Bin
Troja, Eleonora
Yin, Yi-Han Iris
Liu, Yuan
Xiong, Shao-Lin
Xin, Li-Ping
Shao, Yi-Xuan
Yang, Jun
Sun, Hui
Xu, Dong
Yang, Yu-Han
Ricci, Roberto
Gao, He
Antier, Sarah
Becerra, Rosa L.
Cao, Jia-Xin
Castro-Tirado, Alberto Javier
Chen, Xin-Lei
Cheng, Ye-Hao
Chen, Yong
Cheng, Hua-Qing
D'Elia, Valerio
De Pasquale, Massimiliano
Dong, Yong-Wei
Elhosseiny, Eslam
Eyles-Ferris, Rob A. J.
Gritsevich, Maria
Han, Xu-Hui
Hartmann, Dieter
Hu, You-Dong
Hu, Jing-Wei
Jia, Shu-Mei
Kochiashvili, Nino
Lei, Wei-Hua
Levan, Andrew J.
Li, Cheng-Kui
Li, Dong-Yue
Li, Hua-Li
Li, Xiao-Bo
Ling, Zhi-Xing
Liu, He-Yang
Lv, Hou-Jun
Malesani, Daniele B.
O'Connor, Brendan
Pan, Hai-Wu
Pandey, Shashi Bhushan
Perez-Garcia, Ignacio
Pieterse, Daniëlle L. A.
Pillas, Marion
Qiu, Yu-Lei
Saccardi, Andrea
Sánchez-Ramírez, Rubén
Tan, Wen-Jun
Tanasan, Manasanun
Tanvir, Nial R.
Vergani, Susanna D.
Wang, Jing
Wang, Xiao-Feng
Wu, Qin-Yu
Yi, Shu-Xu
Yusufjon, Tillayev
Zhang, Chen
Zhang, Wen-Da
Zhang, Yi-Jia
Zhao, Guo-Ying
Zheng, Chao
Zheng, Shi-Jie
Zhou, Chang
Zhou, Ping
Cordier, Bertrand
Wei, Jian-Yan
Yuan, Weimin
Zhang, Shuang-Nan
Zhang, Bing
author_facet Li, An
Wang, Chen-Wei
Passaleva, Niccolò
An, Jie
Zhang, Bin-Bin
Troja, Eleonora
Yin, Yi-Han Iris
Liu, Yuan
Xiong, Shao-Lin
Xin, Li-Ping
Shao, Yi-Xuan
Yang, Jun
Sun, Hui
Xu, Dong
Yang, Yu-Han
Ricci, Roberto
Gao, He
Antier, Sarah
Becerra, Rosa L.
Cao, Jia-Xin
Castro-Tirado, Alberto Javier
Chen, Xin-Lei
Cheng, Ye-Hao
Chen, Yong
Cheng, Hua-Qing
D'Elia, Valerio
De Pasquale, Massimiliano
Dong, Yong-Wei
Elhosseiny, Eslam
Eyles-Ferris, Rob A. J.
Gritsevich, Maria
Han, Xu-Hui
Hartmann, Dieter
Hu, You-Dong
Hu, Jing-Wei
Jia, Shu-Mei
Kochiashvili, Nino
Lei, Wei-Hua
Levan, Andrew J.
Li, Cheng-Kui
Li, Dong-Yue
Li, Hua-Li
Li, Xiao-Bo
Ling, Zhi-Xing
Liu, He-Yang
Lv, Hou-Jun
Malesani, Daniele B.
O'Connor, Brendan
Pan, Hai-Wu
Pandey, Shashi Bhushan
Perez-Garcia, Ignacio
Pieterse, Daniëlle L. A.
Pillas, Marion
Qiu, Yu-Lei
Saccardi, Andrea
Sánchez-Ramírez, Rubén
Tan, Wen-Jun
Tanasan, Manasanun
Tanvir, Nial R.
Vergani, Susanna D.
Wang, Jing
Wang, Xiao-Feng
Wu, Qin-Yu
Yi, Shu-Xu
Yusufjon, Tillayev
Zhang, Chen
Zhang, Wen-Da
Zhang, Yi-Jia
Zhao, Guo-Ying
Zheng, Chao
Zheng, Shi-Jie
Zhou, Chang
Zhou, Ping
Cordier, Bertrand
Wei, Jian-Yan
Yuan, Weimin
Zhang, Shuang-Nan
Zhang, Bing
contents Compact object mergers are multi-messenger sources and progenitors of some gamma-ray bursts (GRBs), primarily understood by gamma-ray observations, while poorly constrained in the prompt low-energy phase. A long-lasting X-ray emission was discussed as afterglows following several short-duration ($\lesssim$2 s) bursts, yet this prompt X-ray component was not directly observed or confirmed. Here we report the discovery of a minutes-long ($\sim$560 s) flash of soft X-rays immediately following the short ($\sim$0.4 s) GRB 250704B. The long-soft bump points to a distinct phase of prompt emission in X-rays detected by Einstein Probe in an event that otherwise appear as an ordinary short GRB, showing that long-lasting X-ray emission is likely a common feature of merger-driven bursts and a promising electromagnetic counterpart to gravitational-wave sources.
format Preprint
id arxiv_https___arxiv_org_abs_2601_14137
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Minutes-long soft X-ray prompt emission from a compact object merger
Li, An
Wang, Chen-Wei
Passaleva, Niccolò
An, Jie
Zhang, Bin-Bin
Troja, Eleonora
Yin, Yi-Han Iris
Liu, Yuan
Xiong, Shao-Lin
Xin, Li-Ping
Shao, Yi-Xuan
Yang, Jun
Sun, Hui
Xu, Dong
Yang, Yu-Han
Ricci, Roberto
Gao, He
Antier, Sarah
Becerra, Rosa L.
Cao, Jia-Xin
Castro-Tirado, Alberto Javier
Chen, Xin-Lei
Cheng, Ye-Hao
Chen, Yong
Cheng, Hua-Qing
D'Elia, Valerio
De Pasquale, Massimiliano
Dong, Yong-Wei
Elhosseiny, Eslam
Eyles-Ferris, Rob A. J.
Gritsevich, Maria
Han, Xu-Hui
Hartmann, Dieter
Hu, You-Dong
Hu, Jing-Wei
Jia, Shu-Mei
Kochiashvili, Nino
Lei, Wei-Hua
Levan, Andrew J.
Li, Cheng-Kui
Li, Dong-Yue
Li, Hua-Li
Li, Xiao-Bo
Ling, Zhi-Xing
Liu, He-Yang
Lv, Hou-Jun
Malesani, Daniele B.
O'Connor, Brendan
Pan, Hai-Wu
Pandey, Shashi Bhushan
Perez-Garcia, Ignacio
Pieterse, Daniëlle L. A.
Pillas, Marion
Qiu, Yu-Lei
Saccardi, Andrea
Sánchez-Ramírez, Rubén
Tan, Wen-Jun
Tanasan, Manasanun
Tanvir, Nial R.
Vergani, Susanna D.
Wang, Jing
Wang, Xiao-Feng
Wu, Qin-Yu
Yi, Shu-Xu
Yusufjon, Tillayev
Zhang, Chen
Zhang, Wen-Da
Zhang, Yi-Jia
Zhao, Guo-Ying
Zheng, Chao
Zheng, Shi-Jie
Zhou, Chang
Zhou, Ping
Cordier, Bertrand
Wei, Jian-Yan
Yuan, Weimin
Zhang, Shuang-Nan
Zhang, Bing
High Energy Astrophysical Phenomena
Compact object mergers are multi-messenger sources and progenitors of some gamma-ray bursts (GRBs), primarily understood by gamma-ray observations, while poorly constrained in the prompt low-energy phase. A long-lasting X-ray emission was discussed as afterglows following several short-duration ($\lesssim$2 s) bursts, yet this prompt X-ray component was not directly observed or confirmed. Here we report the discovery of a minutes-long ($\sim$560 s) flash of soft X-rays immediately following the short ($\sim$0.4 s) GRB 250704B. The long-soft bump points to a distinct phase of prompt emission in X-rays detected by Einstein Probe in an event that otherwise appear as an ordinary short GRB, showing that long-lasting X-ray emission is likely a common feature of merger-driven bursts and a promising electromagnetic counterpart to gravitational-wave sources.
title Minutes-long soft X-ray prompt emission from a compact object merger
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2601.14137