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The enhanced X-ray Timing and Polarimetry mission – eXTP: an update on its scientific cases, mission profile and development status

  • Shuang Nan Zhang*
  • , Andrea Santangelo
  • , Yupeng Xu
  • , Marco Feroci
  • , Margarita Hernanz
  • , Fangjun Lu
  • , Yong Chen
  • , Hua Feng
  • , Kirpal Nandra
  • , Weichun Jiang
  • , Jiri Svoboda
  • , Søren Brandt
  • , Stéphane Schanne
  • , Jean Zand
  • , Malgorzata Michalska
  • , Enrico Bozzo
  • , Emrah Kalemci
  • , Ivan Agudo
  • , Mahdi Ahangarianabhari
  • , Gabby Aitink-Kroes
  • Giovanni Ambrosi, Filippo Ambrosino, Zhenghua An, Miguel Angel Perez Torres, Matias Antonelli, Andrea Argan, Viktor Babinec, Luca Baldini, Marco Barbera, Coen van Baren, David Baudin, Jörg Bayer, Ronaldo Bellazzini, Pierluigi Bellutti, Bruna Bertucci, Giuseppe Bertuccio, Xingzi Bi, Mirko Boezio, Valter Bonvicini, Walter Bonvicini, Pol Bordas, Alice Borghese, Giacomo Borghi, Florent Bouyjou, Ayhan Bozkurt, Alessandro Brez, Daniele Brienza, Franck Cadoux, Riccardo Campana, Jiewei Cao, Xuelei Cao, Jorge Casares, Elisabetta Cavazzuti, Francesco Ceraudo, Tianxiang Chen, Wen Chen, Can Chen, Yupeng Chen, Xin Chen, Yehai Chen, Jerome Chenevez, Yaodong Cheng, Daniela Cirrincione, Marta Civitani, Min Cong, Francesco Coti Zelati, Weiwei Cui, Tao Cui, Wei Cui, Boyu Dai, Thomas Dauser, Nicolas De Angelis, Barbara De Marco, Alessandra De Rosa, Ettore Del Monte, Sergio Di Cosimo, Sebastian Diebold, Giuseppe Dilillo, Fei Ding, Roman Dohnal, Zefang Dong, Immacolata Donnarumma, Michal Dovciak, Yuanyuan Du, Lorenzo Ducci, Yuri Evangelista, Qingmei Fan, Yannick Favre, Patrícia Ferrés, Emanuele Fiandrini, Francesco Ficorella, Fabio Fuschino, José Luis Gálvez, Na Gao, Min Gao, Yuqiang Ge, Mingyu Ge, Olivier Gevin, Marco Grassi, Yudong Gu, Quanying Gu, Ju Guan, Manuel Guedel, Xingbo Han, Dawei Han, Huilin He, Junwang He, Paul Hedderman, Jan Willem den Herder, Bin Hong, Ander Hormaetxe, Dongjie Hou, Zexun Hu, Hao Hu, Qingbao Hu, Yu Hu, Yue Huang, Jiangjiang Huang, Qiushi Huang, Jia Huo, Richard Hynek, Kazumi Iwasawa, Lucca Izzo, Long Ji, Shumei Jia, Bowen Jiang, Wei Jiang, Jiechen Jiang, Xiaowei Jiang, Yang Jiao, Ge Jin, Fan Jin, Jordi Jose, Vladimir Karas, Thomas Kennedy, Christian Kirsch, Merlin Kole, Martin Komarek, Ingo Kreykenbohm, Lucien Kuiper, Irfan Kuvvetli, Claudio Labanti, Luca Latronico, Phillip Laubert, Tao Li, Longhui Li, Hong Li, Duo Li, Wei Li, Maoshun Li, Gang Li, Xiaobo Li, Chengkui Li, Bing Li, Haibo Li, Hong Liang, Qiuyan Liao, Jinyuan Liao, Olivier Limousin, Yanjian Lin, Manuel Linares, Rui Liu, Yichen Liu, Zhihao Liu, Hongwei Liu, Xiaojing Liu, Xiaohua Liu, Ugo Lo Cicero, Jens Loehring, Giovanni Lombardi, Maximilian Lorenz, Bing Lu, Leonardo Lucchesi, Tao Luo, Laidan Luo, Jia Ma, Xiang Ma, Daniele Macera, Piero Malcovati, Alberto Manfreda, Josep Maria Paredes, Andrea Marinucci, Adrian Martindale, Norbert Meidinger, Filippo Mele, Vasco Mendes, Bin Meng, Martin Merkl, Aline Meuris, Giovanni Miniutti, Massimo Minuti, Alfredo Morbidini, Gianluca Morgante, Fabio Muleri, Riccardo Munini, Lorenzo Mussolin, Barbara Negri, Jianyin Nie, Petr Novák, Witold Nowosielski, Alessio Nuti, Ahmet Onat, Piotr Orleanski, Leonardo Orsini, Roland Ottensamer, Ge Ou, Luigi Pacciani, Stephane Paltani, Teng Pan, Kai Pan, Giovanni Pareschi, Alessandro Patruno, Giancarlo Pepponi, Emanuele Perinati, Raffaele Piazzolla, Antonino Picciotto, Claudio Piemonte, Michele Pinchera, Samuel Pliego, Juri Poutanen, Liqiang Qi, Fazhi Qi, Pengfei Qiang, Fangjian Qiao, Zheng Qiao, Xiangbiao Qiu, Chengbo Qiu, Jinlu Qu, Alexandre Rachevski, Irina Rashevskaia, Nanda Rea, Marc Ribo, Rob de la Rie, Jerome Rodriguez, Pablo Rodríguez Gil, Gloria Sala, Thomas Schanz, Roberto Serafinelli, Carmelo Sgro, Zhengxiang Shen, Lizhi Sheng, Jingyan Shi, Giorgia Sironi, Konrad Skup, Liming Song, Zeyu Song, Jiangbo Song, Gloria Spandre, Daniele Spiga, Yongquan Su, Liang Sun, Müberra Sungur, Libor Svéda, Gianpiero Tagliaferri, Ying Tan, Lian Tao, Denis Tcherniak, Chris Tenzer, Michela Todaro, Laura Tolos, Gabriel Torok, Diego F. Torres, Alessio Trois, Onur Turhan, Phil Uttley, Andrea Vacchi, Enrico Virgilli, Channah Vogel, Dave Walton, Jian Wang, Xianqi Wang, Bo Wang, Langping Wang, Xiaofeng Wang, Dianlong Wang, Yusa Wang, Juan Wang, Hao Wang, Ruijie Wang, Ping Wang, Lingjun Wang, Wenshuai Wang, Tian Wang, Haoyu Wang, Zhanshan Wang, Anna L. Watts, Xiangyang Wen, Jörn Wilms, Berend Winter, Xin Wu, Chao Wu, Zhenyu Wu, Qiong Wu, Kaiji Wu, Hao Xiong, Shaolin Xiong, Wei Xu, Zhao Xu, Jingjing Xu, Xiongwei Xu, Jiadai Xue, Yongqing Yan, Xingtao Yan, Xianghui Yang, Yanji Yang, Xiongtao Yang, Sheng Yang, Jiawei Yang, Yingquan Yang, Shuxu Yi, Yonggao Yu, Ke Yu, Ganluigi Zampa, Nicola Zampa, Silvia Zane, Andrzej A. Zdziarski, Long Zhang, Shu Zhang, Wenda Zhang, Xiaoli Zhang, Zhen Zhang, Jiawei Zhang, Fan Zhang, Ziliang Zhang, Dali Zhang, Honglin Zhang, Aimei Zhang, Tong Zhang, Hongmei Zhang, Juan Zhang, Liang Zhang, Yueting Zhang, Li Zhao, Baosheng Zhao, Zijian Zhao, Xiaofan Zhao, Haisheng Zhao, Xiaoyun Zhao, Shijie Zheng, Yupeng Zhou, Xiaohong Zhou, Jiahuan Zhu, Yuxuan Zhu, Cheng Zhu, Zhencai Zhu, Nicola Zorzi, Frans Zwart
*Bu çalışma için yazışmadan sorumlu yazar
  • CAS - Institute of High Energy Physics
  • University of Tübingen
  • National Institute for Astrophysics
  • National Institute for Nuclear Physics
  • Facultat de Ciències
  • Institute of Space Studies of Catalonia
  • Tsinghua University
  • Max Planck Institute for Extraterrestrial Physics
  • Czech Academy of Sciences
  • Technical University of Denmark
  • CEA/Saclay
  • SRON Netherlands Institute for Space Research
  • Polish Academy of Sciences
  • University of Geneva
  • Sabanci University
  • Instituto de Astrofísica de Andalucía - CSIC
  • Polytechnic University of Milan
  • L. K. Engineering
  • University of Palermo
  • Fondazione Bruno Kessler
  • University of Perugia
  • CAS - Innovation Academy for Microsatellites
  • University of Barcelona
  • Italian Space Agency
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • Instituto de Astrofísica de Canarias
  • University of Udine
  • Osservatorio Astronomico di Brera
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Polytechnic University of Catalonia
  • Harbin Institute of Technology
  • China Aerospace Science and Technology Corporation
  • University of Pavia
  • University of Vienna
  • North Night Vision Technology Co. Ltd
  • Tongji University
  • Sun Yat-Sen University
  • University College London
  • CAS - Shanghai Institute of Microsystem and Information Technology
  • Shanghai Industrial Technology Research Institute
  • ESTEC
  • University of Leicester
  • European Space Astronomy Centre
  • Istanbul Technical University
  • University of Turku
  • Stockholm University
  • CAS - Xi'an Institute of Optics and Precision Mechanics
  • Shanghai University
  • Scientific and Technological Research Council of Turkey
  • Silesian University in Opava
  • University of Amsterdam
  • School of Chemistry and Chemical Engineering, Harbin Institute of Technology
  • Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences

Araştırma çıktısı: Kitap/Rapor/Konferans Bildirisinde BölümKonferans katkısıHakem

17 Atıf (Scopus)

Özet

The enhanced X-ray Timing and Polarimetry mission (eXTP) is a flagship observatory for X-ray timing, spectroscopy and polarimetry developed by an International Consortium. Thanks to its very large collecting area, good spectral resolution and unprecedented polarimetry capabilities, eXTP will explore the properties of matter and the propagation of light in the most extreme conditions found in the Universe. eXTP will, in addition, be a powerful X-ray observatory. The mission will continuously monitor the X-ray sky, and will enable multiwavelength and multi-messenger studies. The mission is currently in phase B, which will be completed in the middle of 2022.

Orijinal dilİngilizce
Ana bilgisayar yayını başlığıSpace Telescopes and Instrumentation 2022
Ana bilgisayar yayını alt yazısıUltraviolet to Gamma Ray
EditörlerJan-Willem A. den Herder, Shouleh Nikzad, Kazuhiro Nakazawa
YayınlayanSPIE
ISBN (Elektronik)9781510653436
DOI'lar
Yayın durumuYayınlandı - 2022
Harici olarak yayınlandıEvet
EtkinlikSpace Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray - Montreal, United States
Süre: 17 Tem 202222 Tem 2022

Yayın serisi

AdıProceedings of SPIE - The International Society for Optical Engineering
Hacim12181
ISSN (Basılı)0277-786X
ISSN (Elektronik)1996-756X

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???event.eventtypes.event.conference???Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray
Ülke/BölgeUnited States
ŞehirMontreal
Periyot17/07/2222/07/22

Bibliyografik not

Publisher Copyright:
© 2022 SPIE. All rights reserved.

Finansman

The Chinese team acknowledges support by the Chinese Academy of Sciences through the Strategic Priority Research Program, Grant No. XDA15020100. The Italian authors acknowledge funding support by the Italian Space Agency (under agreement n. 2020-3-HH.0 and ASI-INAF n.2017-14-H.O) and INFN (project XRO - X-ray Observatories). The Spanish authors acknowledge funding support from the MICIN/AEI grant PID2019-108709GB-I00. The German team acknowledges support from the Bundesministerium für Wirtschaft und Tech-nologie through the Deutsches Zentrum f¨ur Luft-und Raumfahrt e.V. (DLR) under the grant number FKZ 50 OO 1902. The Polish team acknowledges FNP grant POIR.04.04.00-00-5C65/17. The Czech team acknowledges support from the GACR project 21-06825X. The Turkish team acknowledges support from the Turkish Space Agency.

FinansörlerFinansör numarası
Turkish Space Agency
Grantová Agentura České Republiky21-06825X
Fundacja na rzecz Nauki PolskiejPOIR.04.04.00-00-5C65/17
Chinese Academy of SciencesXDA15020100
Bundesministerium für Wirtschaft und Technologie
Deutsches Zentrum für Luft- und RaumfahrtFKZ 50 OO 1902
Agenzia Spaziale Italiana2020-3-HH.0
Ministerio de Ciencia e Innovación
Agencia Estatal de InvestigaciónPID2019-108709GB-I00

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