A2 Vertaisarvioitu katsausartikkeli tieteellisessä lehdessä
Observatory science with eXTP
Tekijät: Zhou, Ping; Mao, Jirong; Zhang, Liang; Patruno, Alessandro; Bozzo, Enrico; Xu, Yanjun; Santangelo, Andrea; Zane, Silvia; Zhang, Shuangnan; Feng, Hua; Cavecchi, Yuri; de Marco, Barbara; Fan, Junhui; Hou, Xian; Jiang, Pengfei; Romano, Patrizia; Sala, Gloria; Tao, Lian; Veledina, Alexandra; Vink, Jacco; Wang, Song; Wang, Junxian; Wang, Yidi; Weng, Shanshan; Wu, Qingwen; Xie, Fei; Zhang, Guobao; Zhang, Jin; Zhao, Zhanhao; Zheng, Shijie; Barua, Samuzal; Chen, Yuehong; Chen, Yupeng; Chen, Shijiang; Chen, Liang; Chen, Yongyun; Cheng, Xin; Chi, Yiheng; Cui, Lang; de Martino, Domitilla; Deng, Wei; Ducci, Lorenzo; Farinelli, Ruben; Feng, Fabo; Ge, Mingyu; Gu, Minfeng; Guo, Hengxiao; Han, Dawei; Hu, Xinke; Huang, Yongfeng; In't Zand, Jean; Ji, Long; Kang, Jialai; Kini, Yves; Li, Panping; Li, Zhaosheng; Liu, Kuan; Liu, Jiren; Liu, Jieying; Lyu, Ming; Marino, Alessio; Markowitz, Alex; Mezcua, Mar; Middleton, Matt; Mou, Guobin; Ng, C. -y.; Papitto, Alessandro; Pei, Zhiyuan; Peng, Jingqiang; Poutanen, Juri; Shui, Qingcang; Simone, Scaringi; Su, Yang; Tan, Ying; Wang, Xilu; Wang, Pengju; Wang, Di; Wang, Fayin; Wang, Junfeng; Wang, Mengye; Wang, Yusong; Wu, Jiancheng; Xiao, Hubing; Xiong, Dingrong; Xu, Xiaojie; Xue, Rui; Yan, Zhen; Yang, Ming; Yang, Chuyuan; Yang, Wenxin; Ye, Wentao; Yu, Zhuoli; Yuan, Yuhai; Zhang, Xiao; Zhang, Lixia; Zhao, Shujie; Zhao, Qingchang; Zheng, Yonggang; Zheng, Wei; Zuo, Wenwen
Kustantaja: Springer Nature
Julkaisuvuosi: 2025
Lehti:SCIENCE CHINA Physics, Mechanics and Astronomy
Artikkelin numero: 119507
Vuosikerta: 68
Numero: 11
ISSN: 1674-7348
eISSN: 1869-1927
DOI: https://doi.org/10.1007/s11433-025-2799-0
Verkko-osoite: https://link.springer.com/article/10.1007/s11433-025-2799-0
Rinnakkaistallenteen osoite: https://arxiv.org/abs/2506.08367v2
Preprintin osoite: https://arxiv.org/abs/2506.08367v1
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.
Julkaisussa olevat rahoitustiedot:
This work was supported by the China’s Space Origins Exploration Program, the National Natural Science Foundation of China (Grant Nos. 12273010, 12333007, 12433004, 12233002, 12373041, and 12422306), the International Partnership Program of Chinese Academy of Sciences (Grant No. 113111KYSB20190020), the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDA15020100), the Spanish MICIU (Grant Nos. PID2021-124581OB-I0, PID2024-155316NB-I00, and 2021SGR00426), the Ramon y Cajal Fellowship (Grant Nos. RYC2021-032718-I, and RYC2018-025950-I), the European Union NextGenerationEU/PRTR, the Spanish MINECO (Grant Nos. PID2022-136828NB-C44, and PID2023-148661NB-I00), the E.U. FEDER Funds, the AGAUR/Generalitat de Catalunya (Grant No. SGR-386/2021), the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)-Projektnummer (Grant No. 549824807), the Programma di Ricerca Fondamentale INAF 2023, the National SKA Program of China (Grant No. 2020SKA0120300), the National Key R&D Program of China (Grant No. 2021YFA0718500), the Xinjiang Tianchi Program, the Hong Kong Government under HKU (Grant No. 17304524), and the Bagui Scholars Program.
