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Observatory science with eXTP

文献类型：期刊论文

作者Zhou, Ping34,35; Mao JR(毛基荣)36; Zhang, Liang37; Patruno, Alessandro38,39; Bozzo, Enrico40; Xu, Yanjun37; Santangelo, Andrea41; Zane, Silvia44; Zhang, Shuangnan37; Feng, Hua37
刊名SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
出版日期2025-09-28
卷号68期号:11
关键词X-ray astronomy X-ray polarimetry stars supernova remnants pulsar wind nebulae cataclysmic variables X-ray binaries ultraluminous X-ray sources active galactic nuclei
ISSN号1674-7348
DOI10.1007/s11433-025-2799-0
产权排序第3完成单位
文献子类Review
英文摘要Scheduled for launch in 2030, the enhanced X-ray Timing and Polarization (eXTP) telescope is a Chinese space-based mission aimed at studying extreme conditions and phenomena in astrophysics. eXTP will feature three main payloads: Spectroscopy Focusing Array (SFA), Polarimetry Focusing Array (PFA), and a Wide-field Camera (W2C). This white paper outlines observatory science, incorporating key scientific advances and instrumental changes since the publication of the previous white paper. We will discuss perspectives of eXTP on the research domains of flare stars, supernova remnants, pulsar wind nebulae, cataclysmic variables, X-ray binaries, ultraluminous X-ray sources, active galactic nucleus (AGN), and pulsar-based positioning and timekeeping.
学科主题天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学
URL标识查看原文
出版地16 DONGHUANGCHENGGEN NORTH ST, BEIJING 100717, PEOPLES R CHINA
WOS关键词X-RAY-EMISSION ; QUASI-PERIODIC ERUPTIONS ; ACTIVE GALACTIC NUCLEI ; MASS BLACK-HOLES ; SPECTRAL ENERGY-DISTRIBUTIONS ; ACTIVITY-ROTATION RELATIONSHIP ; ACCUMULATED DIFFUSIVE PROTONS ; IA SUPERNOVAE DEPENDENCE ; DEEP CHANDRA OBSERVATION ; DISK INSTABILITY MODEL
资助项目China's Space Origins Exploration Program; National Natural Science Foundation of China[12273010]; National Natural Science Foundation of China[12333007]; National Natural Science Foundation of China[12433004]; National Natural Science Foundation of China[12233002]; National Natural Science Foundation of China[12373041]; National Natural Science Foundation of China[12422306]; Strategic Priority Research Program of the Chinese Academy of Sciences[XDA15020100]; International Partnership Program of Chinese Academy of Sciences[113111KYSB20190020]; Spanish MICIU[PID2021-124581OB-I0]; Spanish MICIU[PID2024-155316NB-I00]; Spanish MICIU[2021SGR00426]; Ramon y Cajal Fellowship[RYC2021-032718-I]; Ramon y Cajal Fellowship[RYC2018-025950-I]; European Union NextGenerationEU/PRTR; Spanish MINECO[PID2022-136828NB-C44]; Spanish MINECO[PID2023-148661NB-I00]; E.U. FEDER Funds; AGAUR/Generalitat de Catalunya[SGR-386/2021]; Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)[549824807]; Programma di Ricerca Fondamentale INAF 2023; National SKA Program of China[2020SKA0120300]; National Key R&D Program of China[2021YFA0718500]; Xinjiang Tianchi Program; Hong Kong Government under HKU[17304524]; Bagui Scholars Program
WOS研究方向Physics
语种英语
WOS记录号WOS:001589270900001
出版者SCIENCE PRESS
资助机构China's Space Origins Exploration Program ; National Natural Science Foundation of China[12273010, 12333007, 12433004, 12233002, 12373041, 12422306] ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDA15020100] ; International Partnership Program of Chinese Academy of Sciences[113111KYSB20190020] ; Spanish MICIU[PID2021-124581OB-I0, PID2024-155316NB-I00, 2021SGR00426] ; Ramon y Cajal Fellowship[RYC2021-032718-I, RYC2018-025950-I] ; European Union NextGenerationEU/PRTR ; Spanish MINECO[PID2022-136828NB-C44, PID2023-148661NB-I00] ; E.U. FEDER Funds ; AGAUR/Generalitat de Catalunya[SGR-386/2021] ; Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)[549824807] ; Programma di Ricerca Fondamentale INAF 2023 ; National SKA Program of China[2020SKA0120300] ; National Key R&D Program of China[2021YFA0718500] ; Xinjiang Tianchi Program ; Hong Kong Government under HKU[17304524] ; Bagui Scholars Program
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28628]  
专题云南天文台_恒星物理研究组
通讯作者Zhou, Ping; Mao JR(毛基荣); Zhang, Liang; Patruno, Alessandro; Bozzo, Enrico
作者单位1.Department of Astronomy, Xiamen University, Xiamen, 361005, China;
2.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, China;
3.Department of Physics, Centre for Extragalactic Astronomy, Durham University, South Road, Durham, DH1 3LE, UK;
4.INAF Osservatorio Astronomico di Roma, via Frascati 33, Monteporzio Catone, 00078, Italy;
5.Department of Physics, The University of Hong Kong, Pokfulam Rd, Hong Kong, China;
6.School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UK;
7.Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, Warsaw, 00-716, Poland;
8.School of Physical Science and Technology, Southwest Jiaotong University, Chengdu, 611756, China;
9.Key Laboratory of Stars and Interstellar Medium, Xiangtan University, Xiangtan, 411105, China;
10.Gravitation and Astroparticle Physics Amsterdam Institute, University of Amsterdam, Science Park 904, Amsterdam, 1098 XH 195 196, The Netherlands;
推荐引用方式
GB/T 7714		 Zhou, Ping,Mao JR,Zhang, Liang,et al. Observatory science with eXTP[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2025,68(11).
APA Zhou, Ping.,毛基荣.,Zhang, Liang.,Patruno, Alessandro.,Bozzo, Enrico.,...&Zuo, Wenwen.(2025).Observatory science with eXTP.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,68(11).
MLA Zhou, Ping,et al."Observatory science with eXTP".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 68.11(2025).

入库方式： OAI收割

来源：云南天文台

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