The enhanced X-ray Timing and Polarimetry mission—eXTP

  • Shuang Nan Zhang*
  • , Andrea Santangelo
  • , Marco Feroci
  • , Yu Peng Xu
  • , Fang Jun Lu
  • , Yong Chen
  • , Hua Feng
  • , Shu Zhang
  • , Søren Brandt
  • , Margarita Hernanz
  • , Luca Baldini
  • , Enrico Bozzo
  • , Riccardo Campana
  • , Alessandra De Rosa
  • , Yong Wei Dong
  • , Yuri Evangelista
  • , Vladimir Karas
  • , Norbert Meidinger
  • , Aline Meuris
  • , Kirpal Nandra
  • Teng Pan, Giovanni Pareschi, Piotr Orleanski, Qiu Shi Huang, Stephane Schanne, Giorgia Sironi, Daniele Spiga, Jiri Svoboda, Gianpiero Tagliaferri, Christoph Tenzer, Andrea Vacchi, Silvia Zane, Dave Walton, Zhan Shan Wang, Berend Winter, Xin Wu, Jean J.M. in’ t Zand, Mahdi Ahangarianabhari, Giovanni Ambrosi, Filippo Ambrosino, Marco Barbera, Stefano Basso, Jörg Bayer, Ronaldo Bellazzini, Pierluigi Bellutti, Bruna Bertucci, Giuseppe Bertuccio, Giacomo Borghi, Xue Lei Cao, Franck Cadoux, Riccardo Campana, Francesco Ceraudo, Tian Xiang Chen, Yu Peng Chen, Jerome Chevenez, Marta Civitani, Wei Cui, Wei Wei Cui, Thomas Dauser, Ettore Del Monte, Sergio Di Cosimo, Sebastian Diebold, Victor Doroshenko, Michal Dovciak, Yuan Yuan Du, Lorenzo Ducci, Qing Mei Fan, Yannick Favre, Fabio Fuschino, José Luis Gálvez, Min Gao, Ming Yu Ge, Olivier Gevin, Marco Grassi, Quan Ying Gu, Yu Dong Gu, Da Wei Han, Bin Hong, Wei Hu, Long Ji, Shu Mei Jia, Wei Chun Jiang, Thomas Kennedy, Ingo Kreykenbohm, Irfan Kuvvetli, Claudio Labanti, Luca Latronico, Gang Li, Mao Shun Li, Xian Li, Wei Li, Zheng Wei Li, Olivier Limousin, Hong Wei Liu, Xiao Jing Liu, Bo Lu, Tao Luo, Daniele Macera, Piero Malcovati, Adrian Martindale, Malgorzata Michalska, Bin Meng, Massimo Minuti, Alfredo Morbidini, Fabio Muleri, Stephane Paltani, Emanuele Perinati, Antonino Picciotto, Claudio Piemonte, Jin Lu Qu, Alexandre Rachevski, Irina Rashevskaya, Jerome Rodriguez, Thomas Schanz, Zheng Xiang Shen, Li Zhi Sheng, Jiang Bo Song, Li Ming Song, Carmelo Sgro, Liang Sun, Ying Tan, Phil Uttley, Bo Wang, Dian Long Wang, Guo Feng Wang, Juan Wang, Lang Ping Wang, Yu Sa Wang, Anna L. Watts, Xiang Yang Wen, Jörn Wilms, Shao Lin Xiong, Jia Wei Yang, Sheng Yang, Yan Ji Yang, Nian Yu, Wen Da Zhang, Gianluigi Zampa, Nicola Zampa, Andrzej A. Zdziarski, Ai Mei Zhang, Cheng Mo Zhang, Fan Zhang, Long Zhang, Tong Zhang, Yi Zhang, Xiao Li Zhang, Zi Liang Zhang, Bao Sheng Zhao, Shi Jie Zheng, Yu Peng Zhou, Nicola Zorzi, J. Frans Zwart
*Corresponding author for this work

Research output: Contribution to journalReview articlepeer-review

Abstract

In this paper we present the enhanced X-ray Timing and Polarimetry mission—eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to detect the electro-magnetic counterparts of gravitational wave sources. The paper provides a detailed description of: (1) the technological and technical aspects, and the expected performance of the instruments of the scientific payload; (2) the elements and functions of the mission, from the spacecraft to the ground segment.

Original languageEnglish
Article number29502
JournalScience China: Physics, Mechanics and Astronomy
Volume62
Issue number2
DOIs
StatePublished - 1 Feb 2019

Keywords

  • X-ray instrumentation
  • X-ray polarimetry
  • X-ray timing
  • space mission: eXTP

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