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Science objectives of the Einstein Probe mission
Yuan, Weimin1,2; Dai, Lixin3; Feng, Hua4; Jin, Chichuan1,2; Jonker, Peter5,6; Kuulkers, Erik7; Liu, Yuan1; Nandra, Kirpal8; O'Brien, Paul9; Piro, Luigi10; Rau, Arne8; Rea, Nanda11,12; Sanders, Jeremy8; Tao, Lian4; Wang, Junfeng13; Wu, Xuefeng14,15; Zhang, Bing16,17; Zhang, Shuangnan2,4; Ai, Shunke18; Buchner, Johannes8; Bulbul, Esra8; Chen, Hechao19; Chen, Minghua2,20; Chen, Yong4; Chen, Yu-Peng4; Coleiro, Alexis21; Zelati, Francesco Coti11,12; Dai, Zigao22; Fan, Xilong18; Fan, Zhou1,2; Friedrich, Susanne8; Gao, He23,24; Ge, Chong13; Ge, Mingyu4; Geng, Jinjun14; Ghirlanda, Giancarlo25,26; Gianfagna, Giulia10,27; Gou, Lijun1,2; Guillot, Sebastien28; Hou, Xian29,30; Hu, Jingwei1; Huang, Yongfeng31,32; Ji, Long33; Jia, Shumei2,4; Komossa, S.34; Kong, Albert K. H.35; Lan, Lin1; Li, An23,24; Li, Ang13; Li, Chengkui4; Li, Dongyue1; Li, Jian15,22; Li, Zhaosheng36; Ling, Zhixing1,2; Liu, Ang8; Liu, Jinzhong2,20; Liu, Liangduan37,38; Liu, Zhu8; Luo, Jiawei39,40; Ma, Ruican2,4; Maggi, Pierre41; Maitra, Chandreyee8; Marino, Alessio11,12; Ng, Stephen Chi-Yung3; Pan, Haiwu1; Rukdee, Surangkhana8; Soria, Roberto2,42,43; Sun, Hui1; Tam, Pak-Hin Thomas33; Thakur, Aishwarya Linesh10; Tian, Hui44; Troja, Eleonora10,45; Wang, Wei18; Wang, Xiangyu31; Wang, Yanan1; Wei, Junjie14,15; Wen, Sixiang1; Wu, Jianfeng13; Wu, Ting20; Xiao, Di14,15; Xu, Dong1; Xu, Renxin46,47,48; Xu, Yanjun4; Xu, Yu44; Yang, Haonan1,2; You, Bei18; Yu, Heng24; Yu, Yunwei37,38; Zhang, Binbin14,31,32; Zhang, Chen1,2; Zhang, Guobao29,30; Zhang, Liang4; Zhang, Wenda1; Zhang, Yu2,20; Zhou, Ping31; Zou, Zecheng31,32
2025-03-01
Source PublicationSCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
ISSN1674-7348
Volume68Issue:3Pages:239501
Contribution Rank20
AbstractThe Einstein Probe (EP) is an interdisciplinary mission of time-domain and X-ray astronomy. Equipped with a wide-field lobster-eye X-ray focusing imager, EP will discover cosmic X-ray transients and monitor the X-ray variability of known sources in 0.5-4 keV, at a combination of detecting sensitivity and cadence that is not accessible to the previous and current wide-field monitoring missions. EP can perform quick characterisation of transients or outbursts with a Wolter-I X-ray telescope onboard. In this paper, the science objectives of the EP mission are presented. EP is expected to enlarge the sample of previously known or predicted but rare types of transients with a wide range of timescales. Among them, fast extragalactic transients will be surveyed systematically in soft X-rays, which include gamma-ray bursts and their variants, supernova shock breakouts, and the predicted X-ray transients associated with binary neutron star mergers. EP will detect X-ray tidal disruption events and outbursts from active galactic nuclei, possibly at an early phase of the flares for some. EP will monitor the variability and outbursts of X-rays from white dwarfs, neutron stars and black holes in our and neighbouring galaxies at flux levels fainter than those detectable by the current instruments, and is expected to discover new objects. A large sample of stellar X-ray flares will also be detected and characterised. In the era of multi-messenger astronomy, EP has the potential of detecting the possible X-ray counterparts of gravitational wave events, neutrino sources, and ultra-high energy gamma-ray and cosmic ray sources. EP is expected to help advance the studies of extreme objects and phenomena revealed in the dynamic X-ray universe, and their underlying physical processes. Besides EP's strength in time-domain science, its follow-up telescope, with excellent performance, will also enable advances in many areas of X-ray astronomy.
KeywordEinstein Probe X-ray astronomy X-ray telescopes time-domain astronomy transients variability
DOI10.1007/s11433-024-2600-3
Indexed BySCI
Language英语
WOS KeywordGAMMA-RAY BURSTS ; TIDAL DISRUPTION EVENTS ; QUASI-PERIODIC ERUPTIONS ; ACTIVE GALACTIC NUCLEI ; SUPERMASSIVE BLACK-HOLE ; BLUE OPTICAL TRANSIENT ; CORONAL MASS EJECTION ; CHANGING-LOOK AGN ; EQUATORIAL-DEPTH SURVEY ; HIGH-ENERGY NEUTRINO
Funding ProjectStrategic Priority Program on Space Science of Chinese Academy of Sciences ; Strategic Priority Program on Space Science of Chinese Academy of Sciences ; Strategic Priority Program on Space Science of Chinese Academy of Sciences ; ESA ; ESA ; ESA ; MPE ; MPE ; MPE ; CNES[XDA15310000] ; CNES[XDA15052100] ; CNES ; CNES ; National Natural Science Foundation of China[61234003] ; National Natural Science Foundation of China[61434004] ; National Natural Science Foundation of China[61504141] ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; CAS Interdisciplinary Project[KJZD-EW-L11-04] ; CAS Interdisciplinary Project ; CAS Interdisciplinary Project
WOS Research AreaPhysics
WOS SubjectPhysics, Multidisciplinary
WOS IDWOS:001407830200001
PublisherSCIENCE PRESS
Funding OrganizationStrategic Priority Program on Space Science of Chinese Academy of Sciences ; Strategic Priority Program on Space Science of Chinese Academy of Sciences ; Strategic Priority Program on Space Science of Chinese Academy of Sciences ; ESA ; ESA ; ESA ; MPE ; MPE ; MPE ; CNES ; CNES ; CNES ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; CAS Interdisciplinary Project ; CAS Interdisciplinary Project ; CAS Interdisciplinary Project
Citation statistics
Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/7423
Collection光学天文与技术应用研究室_变星研究团组
光学天文与技术应用研究室_星团与星系研究团组
Corresponding AuthorYuan, Weimin
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
2.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
3.Univ Hong Kong, Dept Phys, Pokfulam Rd, Hong Kong 999077, Peoples R China
4.Chinese Acad Sci, Key Lab Particle Astrophys, Inst High Energy Phys, Beijing 100049, Peoples R China
5.Radboud Univ Nijmegen, Dept Astrophys, IMAPP, NL-6500 GL Nijmegen, Netherlands
6.SRON Netherlands Inst Space Res, NL-2333 CA Leiden, Netherlands
7.ESA ESTEC, NL-2201 AZ Noordwijk, Netherlands
8.Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
9.Univ Leicester, Sch Phys & Astron, Leicester LE1 7RH, England
10.INAF Ist Astrofis & Planetol Spaziali, I-00133 Rome, Italy
11.CSIC, Inst Space Sci ICE, Campus UAB, E-08193 Barcelona, Spain
12.Inst Estudis Espacials Catalunya IEEC, E-08034 Barcelona, Spain
13.Xiamen Univ, Dept Astron, Xiamen 361005, Peoples R China
14.Chinese Acad Sci, Purple Mt Observ, Nanjing 210023, Peoples R China
15.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China
16.Univ Nevada, Nevada Ctr Astrophys, Las Vegas, NV 89154 USA
17.Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
18.Wuhan Univ, Sch Phys & Technol, Dept Astron, Wuhan 430072, Peoples R China
19.Yunnan Univ, Sch Phys & Astron, Kunming 650500, Peoples R China
20.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
21.Univ Paris Cite, CNRS, AstroParticule & Cosmol, F-75013 Paris, France
22.Univ Sci & Technol China, Dept Astron, Hefei 230026, Peoples R China
23.Beijing Normal Univ, Inst Frontier Astron & Astrophys, Beijing 102206, Peoples R China
24.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
25.INAF Osservatorio Astron Brera, I-23807 Merate, LC, Italy
26.INFN Sez Milano Bicocca, I-20126 Milan, MI, Italy
27.Univ Roma Tre, Dipartimento Fis, I-00146 Rome, Italy
28.CNES, Inst Rech Astrophys & Planetol, UPS OMP, CNRS, F-31028 Toulouse, France
29.Chinese Acad Sci, Yunnan Observ, Kunming 650216, Peoples R China
30.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650216, Peoples R China
31.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China
32.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210023, Peoples R China
33.Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519082, Peoples R China
34.Max Planck Inst Radioastron, D-53121 Bonn, Germany
35.Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
36.Xiangtan Univ, Key Lab Stars & Interstellar Medium, Xiangtan 411105, Peoples R China
37.Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China
38.Cent China Normal Univ, Key Lab Quark & Lepton Phys, Minist Educ, Wuhan 430079, Peoples R China
39.Hebei Normal Univ, Coll Phys, Shijiazhuang 050024, Peoples R China
40.Hebei Normal Univ, Hebei Key Lab Photophys Res & Applicat, Shijiazhuang 050024, Peoples R China
41.Univ Strasbourg, Observ Astron Strasbourg, CNRS UMR7550, F-67000 Strasbourg, France
42.INAF Osservatorio Astrofis Torino, I-10025 Pino Torinese, Italy
43.Univ Sydney, Sydney Inst Astron, Sch Phys A28, Sydney, NSW 2006, Australia
44.Peking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
45.Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy
46.Peking Univ, Sch Phys, Beijing 100871, Peoples R China
47.Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China
48.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
Recommended Citation
GB/T 7714
Yuan, Weimin,Dai, Lixin,Feng, Hua,et al. Science objectives of the Einstein Probe mission[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2025,68(3):239501.
APA Yuan, Weimin.,Dai, Lixin.,Feng, Hua.,Jin, Chichuan.,Jonker, Peter.,...&Zou, Zecheng.(2025).Science objectives of the Einstein Probe mission.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,68(3),239501.
MLA Yuan, Weimin,et al."Science objectives of the Einstein Probe mission".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 68.3(2025):239501.
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