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Science objectives of the Einstein Probe mission

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  • Published: 24 January 2025
  • Volume 68, article number 239501, (2025)
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Science objectives of the Einstein Probe mission
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  • Weimin Yuan1,2,
  • Lixin Dai3,
  • Hua Feng4,
  • Chichuan Jin1,2,
  • Peter Jonker5,6,
  • Erik Kuulkers7,
  • Yuan Liu1,
  • Kirpal Nandra8,
  • Paul O’Brien9,
  • Luigi Piro10,
  • Arne Rau8,
  • Nanda Rea11,12,
  • Jeremy Sanders8,
  • Lian Tao4,
  • Junfeng Wang13,
  • Xuefeng Wu14,15,
  • Bing Zhang16,17,
  • Shuangnan Zhang4,2,
  • Shunke Ai18,
  • Johannes Buchner8,
  • Esra Bulbul8,
  • Hechao Chen19,
  • Minghua Chen20,2,
  • Yong Chen4,
  • Yu-Peng Chen4,
  • Alexis Coleiro21,
  • Francesco Coti Zelati11,12,
  • Zigao Dai22,
  • Xilong Fan18,
  • Zhou Fan1,2,
  • Susanne Friedrich8,
  • He Gao23,24,
  • Chong Ge13,
  • Mingyu Ge4,
  • Jinjun Geng14,
  • Giancarlo Ghirlanda25,26,
  • Giulia Gianfagna10,27,
  • Lijun Gou1,2,
  • Sébastien Guillot28,
  • Xian Hou29,30,
  • Jingwei Hu1,
  • Yongfeng Huang31,32,
  • Long Ji33,
  • Shumei Jia4,2,
  • S. Komossa34,
  • Albert K. H. Kong35,
  • Lin Lan1,
  • An Li23,24,
  • Ang Li13,
  • Chengkui Li4,
  • Dongyue Li1,
  • Jian Li22,15,
  • Zhaosheng Li36,
  • Zhixing Ling1,2,
  • Ang Liu8,
  • Jinzhong Liu20,2,
  • Liangduan Liu37,38,
  • Zhu Liu8,
  • Jiawei Luo39,
  • Ruican Ma4,2,
  • Pierre Maggi40,
  • Chandreyee Maitra8,
  • Alessio Marino11,12,
  • Stephen Chi-Yung Ng3,
  • Haiwu Pan1,
  • Surangkhana Rukdee8,
  • Roberto Soria2,41,42,
  • Hui Sun1,
  • Pak-Hin Thomas Tam33,
  • Aishwarya Linesh Thakur10,
  • Hui Tian43,
  • Eleonora Troja44,10,
  • Wei Wang18,
  • Xiangyu Wang31,
  • Yanan Wang1,
  • Junjie Wei14,15,
  • Sixiang Wen1,
  • Jianfeng Wu13,
  • Ting Wu20,
  • Di Xiao14,15,
  • Dong Xu1,
  • Renxin Xu45,46,
  • Yanjun Xu4,
  • Yu Xu43,
  • Haonan Yang1,2,
  • Bei You18,
  • Heng Yu24,
  • Yunwei Yu37,38,
  • Binbin Zhang31,32,14,
  • Chen Zhang1,2,
  • Guobao Zhang29,30,
  • Liang Zhang4,
  • Wenda Zhang1,
  • Yu Zhang20,2,
  • Ping Zhou31 &
  • …
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Abstract

The 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 γ-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 γ-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.

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Authors and Affiliations

  1. National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China

    Weimin Yuan, Chichuan Jin, Yuan Liu, Zhou Fan, Lijun Gou, Jingwei Hu, Lin Lan, Dongyue Li, Zhixing Ling, Haiwu Pan, Hui Sun, Yanan Wang, Sixiang Wen, Dong Xu, Haonan Yang, Chen Zhang & Wenda Zhang

  2. School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Beijing, 100049, China

    Weimin Yuan, Chichuan Jin, Shuangnan Zhang, Minghua Chen, Zhou Fan, Lijun Gou, Shumei Jia, Zhixing Ling, Jinzhong Liu, Ruican Ma, Roberto Soria, Haonan Yang, Chen Zhang & Yu Zhang

  3. Department of Physics, University of Hong Kong, Pokfulam Road, Hong Kong, 999077, China

    Lixin Dai & Stephen Chi-Yung Ng

  4. Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China

    Hua Feng, Lian Tao, Shuangnan Zhang, Yong Chen, Yu-Peng Chen, Mingyu Ge, Shumei Jia, Chengkui Li, Ruican Ma, Yanjun Xu & Liang Zhang

  5. Department of Astrophysics/IMAPP, Radboud University, Nijmegen, 6500 GL, the Netherlands

    Peter Jonker

  6. SRON, Netherlands Institute for Space Research, Leiden, 2333 CA, the Netherlands

    Peter Jonker

  7. ESA/ESTEC, Noordwijk, 2201 AZ, the Netherlands

    Erik Kuulkers

  8. Max Planck Institute for Extraterrestrial Physics, Garching, 85748, Germany

    Kirpal Nandra, Arne Rau, Jeremy Sanders, Johannes Buchner, Esra Bulbul, Susanne Friedrich, Ang Liu, Zhu Liu, Chandreyee Maitra & Surangkhana Rukdee

  9. School of Physics and Astronomy, University of Leicester, Leicester, LE1 7RH, UK

    Paul O’Brien

  10. INAF-Istituto di Astrofisica e Planetologia Spaziali, Rome, 00133, Italy

    Luigi Piro, Giulia Gianfagna, Aishwarya Linesh Thakur & Eleonora Troja

  11. Institute of Space Sciences (ICE), CSIC, Campus UAB, Barcelona, E-08193, Spain

    Nanda Rea, Francesco Coti Zelati & Alessio Marino

  12. Institut d’Estudis Espacials de Catalunya (IEEC), Barcelona, E-08034, Spain

    Nanda Rea, Francesco Coti Zelati & Alessio Marino

  13. Department of Astronomy, Xiamen University, Xiamen, 361005, China

    Junfeng Wang, Chong Ge, Ang Li & Jianfeng Wu

  14. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, China

    Xuefeng Wu, Jinjun Geng, Junjie Wei, Di Xiao & Binbin Zhang

  15. School of Astronomy and Space Sciences, University of Science and Technology of China, Hefei, 230026, China

    Xuefeng Wu, Jian Li, Junjie Wei & Di Xiao

  16. Nevada Center for Astrophysics, University of Nevada, Las Vegas, NV, 89154, USA

    Bing Zhang

  17. Department of Physics and Astronomy, University of Nevada, Las Vegas, NV, 89154, USA

    Bing Zhang

  18. Department of Astronomy, School of Physics and Technology, Wuhan University, Wuhan, 430072, China

    Shunke Ai, Xilong Fan, Wei Wang & Bei You

  19. School of Physics and Astronomy, Yunnan University, Kunming, 650500, China

    Hechao Chen

  20. Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, 830011, China

    Minghua Chen, Jinzhong Liu, Ting Wu & Yu Zhang

  21. CNRS, Astroparticule et Cosmologie, Université Paris Cité, Paris, F-75013, France

    Alexis Coleiro

  22. Department of Astronomy, University of Science and Technology of China, Hefei, 230026, China

    Zigao Dai & Jian Li

  23. Institute for Frontier in Astronomy and Astrophysics, Beijing Normal University, Beijing, 102206, China

    He Gao & An Li

  24. Department of Astronomy, Beijing Normal University, Beijing, 100875, China

    He Gao, An Li & Heng Yu

  25. INAF–Osservatorio Astronomico di Brera, Merate, LC, I-23807, Italy

    Giancarlo Ghirlanda

  26. INFN–sezione di Milano-Bicocca, Milano, MI, I-20126, Italy

    Giancarlo Ghirlanda

  27. Dipartimento di Fisica, Università di Roma “Sapienza”, Roma, I-00185, Italy

    Giulia Gianfagna

  28. Institut de Recherche en Astrophysique et Planétologie, UPS-OMP, CNRS, CNES, Toulouse Cedex 4, F-31028, France

    Sébastien Guillot

  29. Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China

    Xian Hou & Guobao Zhang

  30. Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650216, China

    Xian Hou & Guobao Zhang

  31. School of Astronomy and Space Science, Nanjing University, Nanjing, 210023, China

    Yongfeng Huang, Xiangyu Wang, Binbin Zhang, Ping Zhou & Zecheng Zou

  32. Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, Nanjing, 210023, China

    Yongfeng Huang, Binbin Zhang & Zecheng Zou

  33. School of Physics and Astronomy, Sun Yat-sen University, Zhuhai, 519082, China

    Long Ji & Pak-Hin Thomas Tam

  34. Max-Planck-Institut für Radioastronomie, Bonn, 53121, Germany

    S. Komossa

  35. Institute for Cosmic Ray Research, The University of Tokyo, Kashiwa City, Chiba, 277-8582, Japan

    Albert K. H. Kong

  36. Key Laboratory of Stars and Interstellar Medium, Xiangtan University, Xiangtan, 411105, China

    Zhaosheng Li

  37. Institute of Astrophysics, Central China Normal University, Wuhan, 430079, China

    Liangduan Liu & Yunwei Yu

  38. Key Laboratory of Quark and Lepton Physics, Central China Normal University, Ministry of Education, Wuhan, 430079, China

    Liangduan Liu & Yunwei Yu

  39. College of Physics and Hebei Key Laboratory of Photophysics Research and Application, Hebei Normal University, Shijiazhuang, 050024, China

    Jiawei Luo

  40. Observatoire Astronomique de Strasbourg, Université de Strasbourg, CNRS, Strasbourg, F-67000, France

    Pierre Maggi

  41. INAF–Osservatorio Astrofisico di Torino, Pino Torinese, Turin, I-10025, Italy

    Roberto Soria

  42. Sydney Institute for Astronomy, School of Physics A28, The University of Sydney, Sydney, NSW, 2006, Australia

    Roberto Soria

  43. School of Earth and Space Sciences, Peking University, Beijing, 100871, China

    Hui Tian & Yu Xu

  44. Department of Physics, University of Rome “Tor Vergata”, Rome, I-00133, Italy

    Eleonora Troja

  45. School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing, 100871, China

    Renxin Xu

  46. Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, 100871, China

    Renxin Xu

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Corresponding author

Correspondence to Weimin Yuan.

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Conflict of interest The authors declare that they have no conflict of interest.

Additional information

We would like to thank a large number of colleagues, many of whom are not listed as co-authors of this paper, for stimulating discussions on the science objectives and science cases of the EP mission over the past ten years. EP is a space mission supported by Strategic Priority Program on Space Science of Chinese Academy of Sciences, in collaboration with ESA, MPE and CNES (Grant Nos. XDA15310000, and XDA15052100). This work was supported by the National Natural Science Foundation of China (Grant Nos. 61234003, 61434004, and 61504141), and CAS Interdisciplinary Project (Grant No. KJZD-EW-L11-04). We gratefully acknowledge the China National Astronomical Data Center (NADC), the Astronomical Data Center of the Chinese Academy of Sciences, and the Chinese Virtual Observatory (China-VO) for providing data resources and technical support.

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Yuan, W., Dai, L., Feng, H. et al. Science objectives of the Einstein Probe mission. Sci. China Phys. Mech. Astron. 68, 239501 (2025). https://doi.org/10.1007/s11433-024-2600-3

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  • Received: 21 August 2024

  • Accepted: 09 January 2025

  • Published: 24 January 2025

  • Version of record: 24 January 2025

  • DOI: https://doi.org/10.1007/s11433-024-2600-3

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