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Science objectives of the Einstein Probe mission

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摘要 The Einstein Probe(EP)is an interdisciplinary mission of time-domain and X-ray astronomy.Equipped with a wide-field lobstereye 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 includeγ-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 energyγ-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.
机构地区 National Astronomical Observatories School of Astronomy and Space Sciences Department of Physics Key Laboratory of Particle Astrophysics Department of Astrophysics/IMAPP SRON ESA/ESTEC Max Planck Institute for Extraterrestrial Physics School of Physics and Astronomy INAF-Istituto di Astrofisica e Planetologia Spaziali Institute of Space Sciences(ICE) Institut d’Estudis Espacials de Catalunya(IEEC) Department of Astronomy Purple Mountain Observatory School of Astronomy and Space Sciences Nevada Center for Astrophysics Department of Physics and Astronomy Department of Astronomy School of Physics and Astronomy Xinjiang Astronomical Observatory Universit´e Paris Cit´e Department of Astronomy Institute for Frontier in Astronomy and Astrophysics Department of Astronomy INAF-Osservatorio Astronomico di Brera INFN-sezione di Milano-Bicocca Dipartimento di Fisica Institut de Recherche en Astrophysique et Plan´etologie Yunnan Observatories Key Laboratory for the Structure and Evolution of Celestial Objects School of Astronomy and Space Science Key Laboratory of Modern Astronomy and Astrophysics(Nanjing University) School of Physics and Astronomy Max-Planck-Institut f¨ur Radioastronomie Institute for Cosmic Ray Research Key Laboratory of Stars and Interstellar Medium Institute of Astrophysics Key Laboratory of Quark and Lepton Physics(Central China Normal University) College of Physics and Hebei Key Laboratory of Photophysics Research and Application Observatoire Astronomique de Strasbourg INAF-Osservatorio Astrofisico di Torino Sydney Institute for Astronomy School of Earth and Space Sciences Department of Physics School of Physics and State Key Laboratory of Nuclear Physics and Technology Kavli Institute for Astronomy and Astrophysics
出处 《Science China(Physics,Mechanics & Astronomy)》 2025年第3期1-60,共60页 中国科学:物理学、力学、天文学(英文版)
基金 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) supported by the National Natural Science Foundation of China(Grant Nos.61234003,61434004,and 61504141) CAS Interdisciplinary Project(Grant No.KJZD-EW-L11-04)。
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