Soft X-ray prompt emission from the high-redshift gamma-ray burst EP240315a
Yuan Liu
1
,
Hui Sun
1
,
D. Xu
1, 2
,
D. Svinkin
3
,
J. J. DeLaunay
4
,
N. Tanvir
5
,
He Gao
6, 7
,
C. Zhang
1
,
Yong Chen
8
,
X. F. Wu
9
,
Binbin Zhang
10, 11
,
W. Yuan
1, 12
,
J. An
1, 12
,
Gabriele Bruni
13
,
D. D. Frederiks
3
,
G. Ghirlanda
14, 15
,
J. W. Hu
1
,
A. Li
6, 7
,
Cheng-Kui Li
8
,
J.D. LI
6, 7
,
D. B. Malesani
16, 17, 18
,
L. Piro
13
,
G. Raman
4
,
R. Ricci
19
,
E. Troja
19, 20
,
Susanna D. Vergani
21
,
Qinyu Wu
1, 12
,
Jun Yang
22, 23
,
B. B. Zhang
9, 22, 23
,
Z. P. Zhu
1
,
A. De Ugarte Postigo
24, 25
,
A. G. Demin
3
,
D. Dobie
26, 27, 28
,
Z Fan
1
,
S. Y. Fu
1, 12
,
J. U. Fynbo
16, 17
,
Jin-Jun Geng
9
,
Giulia Gianfagna
13
,
Y.-D. Hu
14
,
Y. F. Huang
22
,
S. Q. JIANG
1, 12
,
Peter G. Jonker
18
,
Y. Julakanti
5
,
J. A. Kennea
4
,
A. A. Kokomov
3
,
E. Kuulkers
29
,
Wei‐Hua Lei
30
,
J K Leung
31, 32, 33
,
A. J. Levan
18
,
D. Y. Li
1
,
Y. Li
9
,
S. P. Littlefair
34
,
X. Liu
1, 12
,
A. L. Lysenko
3
,
Y.-N. Ma
6, 7
,
A. Martin-Carrillo
35
,
P. O’Brien
5
,
Tyler Parsotan
36, 37
,
J. Quirola-Vásquez
18
,
A. V. Ridnaia
3
,
S. Ronchini
4
,
A. Rossi
38
,
D. Mata Sánchez
39, 40
,
Benjamin Schneider
41
,
Rong-Feng Shen
42
,
A. L. Thakur
13
,
A. Tohuvavohu
31, 32
,
M. A. P. Torres
39, 40
,
A. E. Tsvetkova
3, 38, 43
,
M. Ulanov
3
,
Jun-Jie Wei
9
,
D. Xiao
9
,
Yi Han Yin
22, 23
,
M. Bai
44
,
Vadim Burwitz
45
,
Z. M. Cai
46
,
F. S. Chen
47
,
H. -L. Chen
48
,
T. X. Chen
8
,
W. Chen
1, 12
,
Yifan Chen
47
,
Chen Y H
46
,
H. Q. Cheng
1
,
B. Cordier
49
,
Chenzhou Cui
1, 12
,
W. W. Cui
8
,
Y. F. Dai
1
,
Z. G. Dai
50
,
J. Eder
45
,
R. A. J. Eyles
5
,
D. W. Fan
1
,
C. Feldman
5
,
Hua Feng
8
,
Z Feng
44
,
P. Friedrich
45
,
X. Gao
51
,
J.-F. Gonzalez
52
,
J. Guan
8
,
D. W. Han
8
,
J. Han
1
,
Dongjie Hou
8
,
H. B. Hu
1
,
T. Hu
44
,
M. H. Huang
1, 12
,
J. Huo
8
,
I. Hutchinson
5
,
Z. Ji
44
,
S. M. Jia
8
,
Z. Q. Jia
1
,
B.-W. Jiang
53
,
Chichuan Jin
1, 12
,
G. JIN
53
,
J. J. Jin
1
,
A. Keereman
29
,
H Lerman
5
,
J. F. Li
47
,
L. H. Li
53
,
M. S. Li
8
,
W. Li
8
,
Z. D. Li
47
,
T.-Y. Lian
1, 12
,
E. W. Liang
54
,
Z. X. Ling
1, 12
,
C. Z. Liu
8
,
H. Y. Liu
1
,
H. Q. Liu
46
,
Mingjun Liu
1, 12
,
Y.-R. Liu
44
,
F. J. Lu
8
,
H. J. Lü
54
,
L.-D. Luo
8
,
F. L. Ma
44
,
J. Ma
8
,
Jirong Mao
55
,
X. Mao
1, 12
,
M. McHugh
5
,
N. Meidinger
45
,
Kirpal Nandra
45
,
J. P. Osborne
5
,
H. W. Pan
1
,
X. Pan
1
,
Maria Edvige Ravasio
14, 18
,
A. Rau
45
,
N. Rea
56, 57
,
Umer Rehman
22, 23, 58
,
J. S. Sanders
45
,
A. Santovincenzo
29
,
Song Lv
8
,
J. Su
44
,
L. J. Sun
44
,
S. L. Sun
47
,
X. J. Sun
47
,
Y.Y. Tan
44
,
Q J Tang
48
,
Y H Tao
1
,
J. Z. Tong
44
,
C.Y. Wang
59
,
H. Wang
8
,
J Wang
8
,
L. Wang
60
,
W. X. Wang
1
,
Xiaofeng Wang
61
,
X. Y. Wang
22, 23
,
Yilong Wang
1, 12
,
Y. S. Wang
8
,
Daming Wei
9
,
R. Willingale
5
,
S. L. Xiong
44
,
H. T. Xu
44
,
J. J. Xu
8
,
X. P. XU
1, 12
,
Y. F. Xu
1, 12
,
Z. XU
53
,
C B Xue
44
,
Y. L. Xue
47
,
A. L. Yan
47
,
F. Yang
1
,
Haonan Yang
1, 12
,
X T Yang
8
,
Y.J. Yang
8
,
Y. W. YU
62
,
Juan Zhang
8
,
M. Zhang
1
,
Shaofei Zhang
8
,
W. D. Zhang
1
,
W. J. Zhang
1
,
Y. H. Zhang
46
,
Z. Zhang
53
,
Z. L. Zhang
8
,
D. H. Zhao
1
,
H. S. Zhao
8
,
X. F. Zhao
8
,
Z. J. Zhao
8
,
L. X. ZHOU
1
,
Y. L. Zhou
46
,
Y. X. Zhu
8
,
Z.C. Zhu
46
,
Xiaoxiong Zuo
1, 12
2
Altay Astronomical Observatory, Altay, China
|
4
6
14
15
16
Cosmic Dawn Center (DAWN), Copenhagen, Denmark
|
21
26
ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), Hawthorn, Australia
|
27
31
36
49
IRFU/Département d’Astrophysique-AIM, CEA Paris-Saclay, Gif-sur-Yvette, France
|
53
North Night Vision Technology Co. Ltd, Nanjing, China
|
56
Institute of Space Sciences (ICE), Consejo Superior de Investigaciones Cientficas (CSIC), Barcelona, Spain
|
Publication type: Journal Article
Publication date: 2025-01-23
scimago Q1
wos Q1
SJR: 4.006
CiteScore: 22.9
Impact factor: 14.3
ISSN: 23973366
Abstract
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 detection of a GRB triggered in the 0.5–4 keV band by the Wide-field X-ray Telescope (WXT) on board the Einstein Probe (EP) mission, designated as EP240315a, whose bright peak was also detected by the Swift Burst Alert Telescope and Konus-Wind through off-line analyses. At a redshift of z = 4.859, EP240315a showed a much longer and more complicated light curve in the soft-X-ray band than in gamma rays. Benefiting from a large field of view (~3,600°2) and a high sensitivity, EP-WXT captured the earlier engine activation and extended late engine activity through a continuous detection. With a peak X-ray flux at the faint end of previously known high-z GRBs, the detection of EP240315a demonstrates the great potential for EP to study the early universe via GRBs. The death of massive stars has traditionally been discovered by explosive events in the gamma-ray band. Liu et al. show that the sensitive wide-field monitor on board Einstein Probe can reveal a weak soft-X-ray signal much earlier than gamma rays.
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Total citations:
36
Citations from 2024:
35
(97.22%)
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Liu Y. et al. Soft X-ray prompt emission from the high-redshift gamma-ray burst EP240315a // Nature Astronomy. 2025. Vol. 9. No. 4. pp. 564-576.
GOST all authors (up to 50)
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Liu Y. et al. Soft X-ray prompt emission from the high-redshift gamma-ray burst EP240315a // Nature Astronomy. 2025. Vol. 9. No. 4. pp. 564-576.
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@article{2025_Liu,
author = {Yuan Liu and Hui Sun and D. Xu and D. Svinkin and J. J. DeLaunay and N. Tanvir and He Gao and C. Zhang and Yong Chen and X. F. Wu and Binbin Zhang and W. Yuan and J. An and Gabriele Bruni and D. D. Frederiks and G. Ghirlanda and J. W. Hu and A. Li and Cheng-Kui Li and J.D. LI and D. B. Malesani and L. Piro and G. Raman and R. Ricci and E. Troja and Susanna D. Vergani and Qinyu Wu and Jun Yang and B. B. Zhang and Z. P. Zhu and A. De Ugarte Postigo and A. G. Demin and D. Dobie and Z Fan and S. Y. Fu and J. U. Fynbo and Jin-Jun Geng and Giulia Gianfagna and Y.-D. Hu and Y. F. Huang and S. Q. JIANG and Peter G. Jonker and Y. Julakanti and J. A. Kennea and A. A. Kokomov and E. Kuulkers and Wei‐Hua Lei and J K Leung and A. J. Levan and D. Y. Li and others},
title = {Soft X-ray prompt emission from the high-redshift gamma-ray burst EP240315a},
journal = {Nature Astronomy},
year = {2025},
volume = {9},
publisher = {Springer Nature},
month = {jan},
url = {https://www.nature.com/articles/s41550-024-02449-8},
number = {4},
pages = {564--576},
doi = {10.1038/s41550-024-02449-8}
}
Cite this
MLA
Copy
Liu, Yuan, et al. “Soft X-ray prompt emission from the high-redshift gamma-ray burst EP240315a.” Nature Astronomy, vol. 9, no. 4, Jan. 2025, pp. 564-576. https://www.nature.com/articles/s41550-024-02449-8.
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