XAO OpenIR
Soft X-ray prompt emission from the high-redshift gamma-ray burst EP240315a
Liu, Y.1; Sun, H.1; Xu, D.1,2; Svinkin, D. S.3; Delaunay, J.4; Tanvir, N. R.5; Gao, H.6,7; Zhang, C.1; Chen, Y.8; Wu, X-F9; Zhang, B.10,11; Yuan, W.1,12; An, J.1,12; Bruni, G.13; Frederiks, D. D.3; Ghirlanda, G.14,15; Hu, J-W1; Li, A.6,7; Li, C-K8; Li, J-D6,7; Malesani, D. B.16,17,18; Piro, L.13; Raman, G.4; Ricci, R.19; Troja, E.19,20; Vergani, S. D.21; Wu, Q-Y1,12; Yang, J.22,23; Zhang, B-B9,22,23; Zhu, Z-P1; Postigo, A. de Ugarte24,25; Demin, A. G.3; Dobie, D.26,27,28; Fan, Z.1; Fu, S-Y1,12; Fynbo, J. P. U.16,17; Geng, J-J9; Gianfagna, G.13; Hu, Y-D14; Huang, Y-F22; Jiang, S-Q1,12; Jonker, P. G.18; Julakanti, Y.5; Kennea, J. A.4; Kokomov, A. A.3; Kuulkers, E.29; Lei, W-H30; Leung, J. K.31,32,33; Levan, A. J.18; Li, D-Y1; Li, Y.9; Littlefair, S. P.34; Liu, X.1,12; Lysenko, A. L.3; Ma, Y-N6,7; Martin-Carrillo, A.35,36; O'Brien, P.5; Parsotan, T.37,38; Quirola-Vasquez, J.18; Ridnaia, A. V.3; Ronchini, S.4; Rossi, A.39; Mata-Sanchez, D.40,41; Schneider, B.42; Shen, R-F43; Thakur, A. L.13; Tohuvavohu, A.31,32; Torres, M. A. P.40,41; Tsvetkova, A. E.3,39,44; Ulanov, M. V.3; Wei, J-J9; Xiao, D.9; Yin, Y-H I.22,23; Bai, M.45; Burwitz, V.46; Cai, Z-M47; Chen, F-S48; Chen, H-L49; Chen, T-X8; Chen, W.1,12; Chen, Y-F48; Chen, Y-H47; Cheng, H-Q1; Cordier, B.50; Cui, C-Z1,12; Cui, W-W8; Dai, Y-F1; Dai, Z-G51; Eder, J.46; Eyles-Ferris, R. A. J.5; Fan, D-W1; Feldman, C.5; Feng, H.8; Feng, Z.45; Friedrich, P.46; Gao, X.52; Gonzalez, J. -F.53; Guan, J.8; Han, D-W8; Han, J.1; Hou, D-J8; Hu, H-B1; Hu, T.45; Huang, M-H1,12; Huo, J.8; Hutchinson, I.5; Ji, Z.45; Jia, S-M8; Jia, Z-Q1; Jiang, B-W54; Jin, C-C1,12; Jin, G.54; Jin, J-J1; Keereman, A.29; Lerman, H.5; Li, J-F48; Li, L-H54; Li, M-S8; Li, W.8; Li, Z-D48; Lian, T-Y1,12; Liang, E-W55; Ling, Z-X1,12; Liu, C-Z8; Liu, H-Y1; Liu, H-Q47; Liu, M-J1,12; Liu, Y-R45; Lu, F-J8; Lu, H-J55; Luo, L-D8; Ma, F. L.45; Ma, J.8; Mao, J-R56; Mao, X.1,12; McHugh, M.5; Meidinger, N.46; Nandra, K.46; Osborne, J. P.5; Pan, H-W1; Pan, X.1; Ravasio, M. E.14,18; Rau, A.46; Rea, N.57,58; Rehman, U.22,23,59; Sanders, J.46; Santovincenzo, A.29; Song, L-M8; Su, J.45; Sun, L-J45; Sun, S-L48; Sun, X-J48; Tan, Y-Y45; Tang, Q-J49; Tao, Y-H1; Tong, J-Z45; Wang, C-Y60; Wang, H.8; Wang, J.8; Wang, L.61; Wang, W-X1; Wang, X-F62; Wang, X-Y22,23; Wang, Y-L1,12; Wang, Y-S8; Wei, D-M9; Willingale, R.5; Xiong, S-L45; Xu, H-T45; Xu, J-J8; Xu, X-P1,12; Xu, Y-F1,12; Xu, Z.54; Xue, C-B45; Xue, Y-L48; Yan, A-L48; Yang, F.1; Yang, H-N1,12; Yang, X-T8; Yang, Y-J8; Yu, Y-W63; Zhang, J.8; Zhang, M.1; Zhang, S-N8; Zhang, W-D1; Zhang, W-J1; Zhang, Y-H47; Zhang, Z.1,12; Zhang, Z.54; Zhang, Z-L8; Zhao, D-H1; Zhao, H-S8; Zhao, X-F8; Zhao, Z-J8; Zhou, L-X1; Zhou, Y-L47; Zhu, Y-X8; Zhu, Z-C47; Zuo, X-X1,12; Liu, Y.64; Sun, H.64; Xu, D.64,65; Svinkin, D. S.66; Delaunay, J.67; Tanvir, N. R.68; Gao, H.69,70; Zhang, C.64; Chen, Y.71; Wu, X-F72; Zhang, B.73,74; Yuan, W.64,75; An, J.64,75; Bruni, G.76; Frederiks, D. D.66; Ghirlanda, G.77,78; Hu, J-W64; Li, A.69,70; Li, C-K71; Li, J-D69,70; Malesani, D. B.79,80,81; Piro, L.76; Raman, G.67; Ricci, R.82; Troja, E.82,83; Vergani, S. D.84; Wu, Q-Y64,75; Yang, J.85,86; Zhang, B-B72,85,86; Zhu, Z-P64; Postigo, A. de Ugarte87,88; Demin, A. G.66; Dobie, D.89,90,91; Fan, Z.64; Fu, S-Y64,75; Fynbo, J. P. U.79,80; Geng, J-J72; Gianfagna, G.76; Hu, Y-D77; Huang, Y-F85; Jiang, S-Q64,75; Jonker, P. G.81; Julakanti, Y.68; Kennea, J. A.67; Kokomov, A. A.66; Kuulkers, E.92; Lei, W-H93; Leung, J. K.94,95,96; Levan, A. J.81; Li, D-Y64; Li, Y.72; Littlefair, S. P.97; Liu, X.64,75; Lysenko, A. L.66; Ma, Y-N69,70; Martin-Carrillo, A.98,99; O'Brien, P.68; Parsotan, T.100,101; Quirola-Vasquez, J.81; Ridnaia, A. V.66; Ronchini, S.67; Rossi, A.102; Mata-Sanchez, D.103,104; Schneider, B.105; Shen, R-F106; Thakur, A. L.76; Tohuvavohu, A.94,95; Torres, M. A. P.103,104; Tsvetkova, A. E.66,102,107; Ulanov, M. V.66; Wei, J-J72; Xiao, D.72; Yin, Y-H I.85,86; Bai, M.108; Burwitz, V.109; Cai, Z-M110; Chen, F-S111; Chen, H-L112; Chen, T-X71; Chen, W.64,75; Chen, Y-F111; Chen, Y-H110; Cheng, H-Q64; Cordier, B.113; Cui, C-Z64,75; Cui, W-W71; Dai, Y-F64; Dai, Z-G114; Eder, J.109; Eyles-Ferris, R. A. J.68; Fan, D-W64; Feldman, C.68; Feng, H.71; Feng, Z.108; Friedrich, P.109; Gao, X.115; Gonzalez, J. -F.116; Guan, J.71; Han, D-W71; Han, J.64; Hou, D-J71; Hu, H-B64; Hu, T.108; Huang, M-H64,75; Huo, J.71; Hutchinson, I.68; Ji, Z.108; Jia, S-M71; Jia, Z-Q64; Jiang, B-W117; Jin, C-C64,75; Jin, G.117; Jin, J-J64; Keereman, A.92; Lerman, H.68; Li, J-F111; Li, L-H117; Li, M-S71; Li, W.71; Li, Z-D111; Lian, T-Y64,75; Liang, E-W118; Ling, Z-X64,75; Liu, C-Z71; Liu, H-Y64; Liu, H-Q110; Liu, M-J64,75; Liu, Y-R108; Lu, F-J71; Lu, H-J118; Luo, L-D71; Ma, F. L.108; Ma, J.71; Mao, J-R119; Mao, X.64,75; McHugh, M.68; Meidinger, N.109; Nandra, K.109; Osborne, J. P.68; Pan, H-W64; Pan, X.64; Ravasio, M. E.77,81; Rau, A.109; Rea, N.120,121; Rehman, U.85,86,122; Sanders, J.109; Santovincenzo, A.92; Song, L-M71; Su, J.108; Sun, L-J108; Sun, S-L111; Sun, X-J111; Tan, Y-Y108; Tang, Q-J112; Tao, Y-H64; Tong, J-Z108; Wang, C-Y123; Wang, H.71; Wang, J.71; Wang, L.124; Wang, W-X64; Wang, X-F125; Wang, X-Y85,86; Wang, Y-L64,75; Wang, Y-S71; Wei, D-M72; Willingale, R.68; Xiong, S-L108; Xu, H-T108; Xu, J-J71; Xu, X-P64,75; Xu, Y-F64,75; Xu, Z.117; Xue, C-B108; Xue, Y-L111; Yan, A-L111; Yang, F.64; Yang, H-N64,75; Yang, X-T71; Yang, Y-J71; Yu, Y-W126; Zhang, J.71; Zhang, M.64; Zhang, S-N71; Zhang, W-D64; Zhang, W-J64; Zhang, Y-H110; Zhang, Z.64,75; Zhang, Z.117; Zhang, Z-L71; Zhao, D-H64; Zhao, H-S71; Zhao, X-F71; Zhao, Z-J71; Zhou, L-X64; Zhou, Y-L110; Zhu, Y-X71; Zhu, Z-C110; Zuo, X-X64,75
2025-01-23
Source PublicationNATURE ASTRONOMY
ISSN2397-3366
Pages14
Contribution Rank51
AbstractLong 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 (similar to 3,600 degrees(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.
Corresponding AuthorGao, H.(gaohe@bnu.edu.cn) ; Zhang, C.(chzhang@bao.ac.cn) ; Chen, Y.(ychen@ihep.ac.cn) ; Wu, X-F(xfwu@pmo.ac.cn)
DOI10.1038/s41550-024-02449-8
Indexed BySCI
Language英语
WOS KeywordSTAR-FORMATION RATE ; LIGHT CURVES ; GRB 090423 ; SWIFT ; AFTERGLOW ; EVOLUTION ; CALIBRATION ; SUPERNOVA ; FLARES ; WIND
Funding ProjectStrategic Priority Program on Space Science of Chinese Academy of Sciences ; European Space Agency ; Max Planck Institute for Extraterrestrial Physics[XDA15310000] ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0550200] ; National Key R&D Program of China[2022YFF0711500] ; National Natural Science Foundation of China[12321003] ; National Natural Science Foundation of China[12103065] ; National Natural Science Foundation of China[12333004] ; National Natural Science Foundation of China[12373040] ; National Natural Science Foundation of China[12021003] ; China Manned Space Project[CMS-CSST-2021-A13] ; China Manned Space Project[CMS-CSST-2021-B11] ; Youth Innovation Promotion Association of the Chinese Academy of Sciences[Y2022026] ; Youth Innovation Promotion Association of the Chinese Academy of Sciences[2023331] ; Chinese Virtual Observatory[68-811] ; Chinese Virtual Observatory[68-020] ; Chinese Virtual Observatory[A47TAC 42] ; Chinese Virtual Observatory[IT-2023B-020] ; Chinese Virtual Observatory[FFUG-2024-0002] ; Accordo ASI e INAF[HERMES 2022-25-HH.0] ; European Research Council (ERC) under the European Union[101095973] ; ERC under the European Union[101002761] ; European Union[AHEAD2020] ; European Union[871158] ; ASI (Italian Space Agency)[2019-27-HH.0] ; ASI (Italian Space Agency)[ST/W000857/1] ; NASA[NAS5-0136] ; European Union (ERC)[101071865] ; Danish National Research Foundation[DNRF140] ; INAF through the GRAWITA Large Program Grant[1.05.12.01.04] ; Spanish Ministry of Science via the Plan de Generacion de Conocimiento[PID2020-120323GB-I00] ; Spanish Ministry of Science via the Plan de Generacion de Conocimiento[PID2021-124879NB-I00] ; PRIN-MIUR[20179ZF5KS] ; Xinjiang Tianchi Program
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001439582700001
PublisherNATURE PORTFOLIO
Funding OrganizationStrategic Priority Program on Space Science of Chinese Academy of Sciences ; European Space Agency ; Max Planck Institute for Extraterrestrial Physics ; Strategic Priority Research Program of the Chinese Academy of Sciences ; National Key R&D Program of China ; National Natural Science Foundation of China ; China Manned Space Project ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Chinese Virtual Observatory ; Accordo ASI e INAF ; European Research Council (ERC) under the European Union ; ERC under the European Union ; European Union ; ASI (Italian Space Agency) ; NASA ; European Union (ERC) ; Danish National Research Foundation ; INAF through the GRAWITA Large Program Grant ; Spanish Ministry of Science via the Plan de Generacion de Conocimiento ; PRIN-MIUR ; Xinjiang Tianchi Program
Citation statistics
Cited Times:8[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/7500
Collection中国科学院新疆天文台
Corresponding AuthorGao, H.; Zhang, C.; Chen, Y.; Wu, X-F; Gao, H.; Zhang, C.; Chen, Y.; Wu, X-F
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
2.Altay Astron Observ, Altay, Peoples R China
3.Ioffe Inst, St Petersburg, Russia
4.Penn State Univ, Dept Astron & Astrophys, University Pk, PA USA
5.Univ Leicester, Sch Phys & Astron, Leicester, Leics, England
6.Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing, Peoples R China
7.Beijing Normal Univ, Dept Astron, Beijing, Peoples R China
8.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing, Peoples R China
9.Chinese Acad Sci, Purple Mt Observ, Nanjing, Peoples R China
10.Univ Nevada, Nevada Ctr Astrophys, Las Vegas, NV USA
11.Univ Nevada, Dept Phys & Astron, Las Vegas, NV USA
12.Univ Chinese Acad Sci, Chinese Acad Sci, Sch Astron & Space Sci, Beijing, Peoples R China
13.Ist Astrofis & Planetol Spaziali, INAF, Rome, Italy
14.Osserv Astron Brera, INAF, Merate, Italy
15.Ist Nazl Fis Nucl, Sez Milano Bicocca, Milan, Italy
16.Cosm Dawn Ctr DAWN, Copenhagen, Denmark
17.Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark
18.Radboud Univ Nijmegen, Dept Astrophys, IMAPP, Nijmegen, Netherlands
19.Univ Roma Tor Vergata, Dept Phys, Rome, Italy
20.INAF, Rome, Italy
21.Univ PSL, Observ Paris, CNRS, GEPI, Meudon, France
22.Nanjing Univ, Sch Astron & Space Sci, Nanjing, Peoples R China
23.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing, Peoples R China
24.Univ Cote Azur, CNRS, Artemis, Observ Cote Azur, Nice, France
25.Aix Marseille Univ, LAM, CNRS, Marseille, France
26.ARC Ctr Excellence Gravitat Wave Discovery OzGrav, Hawthorn, Vic, Australia
27.Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic, Australia
28.Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW, Australia
29.European Space Agcy, Estec, Noordwijk, Netherlands
30.Huazhong Univ Sci & Technol, Dept Astron, Sch Phys, Wuhan, Peoples R China
31.Univ Toronto, David A Dunlap Dept Astron & Astrophys, Toronto, ON, Canada
32.Univ Toronto, Dunlap Inst Astron & Astrophys, Toronto, ON, Canada
33.Hebrew Univ Jerusalem, Racah Inst Phys, Jerusalem, Israel
34.Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England
35.Univ Coll Dublin, Sch Phys, Dublin, Ireland
36.Univ Coll Dublin, Ctr Space Res, Dublin, Ireland
37.Univ Maryland Baltimore Cty, Ctr Space Sci & Technol, Baltimore, MD USA
38.NASA, Astrophys Sci Div, Goddard Space Flight Ctr, Greenbelt, MD USA
39.Osservatorio Astrofis & Sci Spazio, INAF, Bologna, Italy
40.Inst Astrofis Canarias, Santa Cruz De Tenerife, Spain
41.Univ La Laguna, Dept Astrofis, San Cristobal la Laguna, Spain
42.MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA USA
43.Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai, Peoples R China
44.Univ Cagliari, Dept Phys, Monserrato, Italy
45.Chinese Acad Sci, Natl Space Sci Ctr, Beijing, Peoples R China
46.Max Planck Inst Extraterr Phys, Garching, Germany
47.Chinese Acad Sci, Innovat Acad Microsatellites, Shanghai, Peoples R China
48.Chinese Acad Sci, Shanghai Inst Tech Phys, Shanghai, Peoples R China
49.Chinese Acad Sci, Key Lab Technol Space Energy Convers, Tech Inst Phys & Chem, Beijing, Peoples R China
50.CEA Paris Saclay, Dept Astrophys AIM, IRFU, Gif Sur Yvette, France
51.Univ Sci & Technol China, Dept Astron, Sch Phys Sci, Hefei, Peoples R China
52.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi, Peoples R China
53.Univ Claude Bernard Lyon 1, Univ Lyon, CNRS, ENS Lyon,Ctr Rech Astrophys Lyon,UMR5574, St Genis Laval, France
54.North Night Vis Technol Co Ltd, Nanjing, Peoples R China
55.Guangxi Univ, Sch Phys Sci & Technol, Guangxi Key Lab Relativist Astrophys, Nanning, Peoples R China
56.Chinese Acad Sci, Yunnan Observ, Kunming, Yunnan, Peoples R China
57.CSIC, Inst Space Sci ICE, Barcelona, Spain
58.Inst Estudis Espacials Catalunya, Barcelona, Spain
59.Air Univ Islamabad, Dept Phys, Islamabad, Pakistan
60.Tsinghua Univ, Dept Astron, Beijing, Peoples R China
61.Chinese Acad Sci, Ins Elect Engn, Beijing, Peoples R China
62.Tsinghua Univ, Dept Phys, Beijing, Peoples R China
63.Cent China Normal Univ, Inst Astrophys, Wuhan, Peoples R China
64.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
65.Altay Astron Observ, Altay, Peoples R China
66.Ioffe Inst, St Petersburg, Russia
67.Penn State Univ, Dept Astron & Astrophys, University Pk, PA USA
68.Univ Leicester, Sch Phys & Astron, Leicester, Leics, England
69.Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing, Peoples R China
70.Beijing Normal Univ, Dept Astron, Beijing, Peoples R China
71.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing, Peoples R China
72.Chinese Acad Sci, Purple Mt Observ, Nanjing, Peoples R China
73.Univ Nevada, Nevada Ctr Astrophys, Las Vegas, NV USA
74.Univ Nevada, Dept Phys & Astron, Las Vegas, NV USA
75.Univ Chinese Acad Sci, Chinese Acad Sci, Sch Astron & Space Sci, Beijing, Peoples R China
76.Ist Astrofis & Planetol Spaziali, INAF, Rome, Italy
77.Osserv Astron Brera, INAF, Merate, Italy
78.Ist Nazl Fis Nucl, Sez Milano Bicocca, Milan, Italy
79.Cosm Dawn Ctr DAWN, Copenhagen, Denmark
80.Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark
81.Radboud Univ Nijmegen, Dept Astrophys, IMAPP, Nijmegen, Netherlands
82.Univ Roma Tor Vergata, Dept Phys, Rome, Italy
83.INAF, Rome, Italy
84.Univ PSL, Observ Paris, CNRS, GEPI, Meudon, France
85.Nanjing Univ, Sch Astron & Space Sci, Nanjing, Peoples R China
86.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing, Peoples R China
87.Univ Cote Azur, CNRS, Artemis, Observ Cote Azur, Nice, France
88.Aix Marseille Univ, LAM, CNRS, Marseille, France
89.ARC Ctr Excellence Gravitat Wave Discovery OzGrav, Hawthorn, Vic, Australia
90.Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic, Australia
91.Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW, Australia
92.European Space Agcy, Estec, Noordwijk, Netherlands
93.Huazhong Univ Sci & Technol, Dept Astron, Sch Phys, Wuhan, Peoples R China
94.Univ Toronto, David A Dunlap Dept Astron & Astrophys, Toronto, ON, Canada
95.Univ Toronto, Dunlap Inst Astron & Astrophys, Toronto, ON, Canada
96.Hebrew Univ Jerusalem, Racah Inst Phys, Jerusalem, Israel
97.Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England
98.Univ Coll Dublin, Sch Phys, Dublin, Ireland
99.Univ Coll Dublin, Ctr Space Res, Dublin, Ireland
100.Univ Maryland Baltimore Cty, Ctr Space Sci & Technol, Baltimore, MD USA
101.NASA, Astrophys Sci Div, Goddard Space Flight Ctr, Greenbelt, MD USA
102.Osservatorio Astrofis & Sci Spazio, INAF, Bologna, Italy
103.Inst Astrofis Canarias, Santa Cruz De Tenerife, Spain
104.Univ La Laguna, Dept Astrofis, San Cristobal la Laguna, Spain
105.MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA USA
106.Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai, Peoples R China
107.Univ Cagliari, Dept Phys, Monserrato, Italy
108.Chinese Acad Sci, Natl Space Sci Ctr, Beijing, Peoples R China
109.Max Planck Inst Extraterr Phys, Garching, Germany
110.Chinese Acad Sci, Innovat Acad Microsatellites, Shanghai, Peoples R China
111.Chinese Acad Sci, Shanghai Inst Tech Phys, Shanghai, Peoples R China
112.Chinese Acad Sci, Key Lab Technol Space Energy Convers, Tech Inst Phys & Chem, Beijing, Peoples R China
113.CEA Paris Saclay, Dept Astrophys AIM, IRFU, Gif Sur Yvette, France
114.Univ Sci & Technol China, Dept Astron, Sch Phys Sci, Hefei, Peoples R China
115.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi, Peoples R China
116.Univ Claude Bernard Lyon 1, Univ Lyon, CNRS, ENS Lyon,Ctr Rech Astrophys Lyon,UMR5574, St Genis Laval, France
117.North Night Vis Technol Co Ltd, Nanjing, Peoples R China
118.Guangxi Univ, Sch Phys Sci & Technol, Guangxi Key Lab Relativist Astrophys, Nanning, Peoples R China
119.Chinese Acad Sci, Yunnan Observ, Kunming, Yunnan, Peoples R China
120.CSIC, Inst Space Sci ICE, Barcelona, Spain
121.Inst Estudis Espacials Catalunya, Barcelona, Spain
122.Air Univ Islamabad, Dept Phys, Islamabad, Pakistan
123.Tsinghua Univ, Dept Astron, Beijing, Peoples R China
124.Chinese Acad Sci, Ins Elect Engn, Beijing, Peoples R China
125.Tsinghua Univ, Dept Phys, Beijing, Peoples R China
126.Cent China Normal Univ, Inst Astrophys, Wuhan, Peoples R China
Recommended Citation
GB/T 7714
Liu, Y.,Sun, H.,Xu, D.,et al. Soft X-ray prompt emission from the high-redshift gamma-ray burst EP240315a[J]. NATURE ASTRONOMY,2025:14.
APA Liu, Y..,Sun, H..,Xu, D..,Svinkin, D. S..,Delaunay, J..,...&Zuo, X-X.(2025).Soft X-ray prompt emission from the high-redshift gamma-ray burst EP240315a.NATURE ASTRONOMY,14.
MLA Liu, Y.,et al."Soft X-ray prompt emission from the high-redshift gamma-ray burst EP240315a".NATURE ASTRONOMY (2025):14.
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