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EXTP: Enhanced X-ray Timing and Polarization mission
Zhang, S. N.1; Feroci, M.2,58; Santangelo, A.1,3; Dong, Y. W.1; Feng, H.9; Lu, F. J.1; Nandra, K.15; Wang, Z. S.10; Zhang, S.1; Bozzo, E.4; Brandt, S.5; De Rosa, A.2; Gou, L. J.11; Hernanz, M.6; Van Der Klis, M.20; Li, X. D.13; Liu, Y.1; Orleanski, P.26; Pareschi, G.24; Pohl, M.7; Poutanen, J.42; Qu, J. L.1; Schanne, S.40; Stella, L.19; Uttley, P.20; Watts, A.20; Xu, R. X.16; Yu, W. F.12; In't Zand, J. J. M.21; Zane, S.8; Alvarez, L.6; Amati, L.32; Baldini, L.36; Bambi, C.17; Basso, S.24; Bhattacharyya, S.47; Bellazzini, R.36; Belloni, T.24; Bellutti, P.8; Bianchi, S.38; Brez, A.36; Bursa, M.44; Burwitz, V.15; Budtz-Jorgensen, C.5; Caiazzo, I.28; Campana, R.32; Cao, X. L.1; Casella, P.19; Chen, C. Y.54; Chen, L.12; Chen, T. X.1; Chen, Y.1; Chen, Y.13; Chen, Y. P.1; Civitani, M.24; Zelati, F. Coti20,24,52; Cui, W.14,60; Cui, W. W.1; Dai, Z. G.13; Del Monte, E.2,58; De Martino, D.48; Di Cosimo, S.2; Diebold, S.3; Dovciak, M.44; Donnarumma, I.2; Doroshenko, V.3; Esposito, P.34; Evangelista, Y.2,58; Favre, Y.7; Friedrich, P.15; Fuschino, F.32; Galvez, J. L.6; Gao, Z. L.56; Ge, M. Y.1; Gevin, O.40; Goetz, D.40; Han, D. W.1; Heyl, J.28; Horak, J.44; Hu, W.1; Huang, F.54; Huang, Q. S.10; Hudec, R.44,45; Huppenkothen, D.37; Israel, G. L.19; Ingram, A.20; Karas, V.44; Karelin, D.6; Jenke, P. A.; Ji, L.1; Kennedy, T.8; Korpela, S.41; Kunneriath, D.44; Labanti, C.32; Li, G.1; Li, X.1; Li, Z. S.29; Liang, E. W.58; Limousin, O.40; Lin, L.31; Ling, Z. X.11; Liu, H. B.58; Liu, H. W.1; Liu, Z.11; Lu, B.1; Lund, N.5; Lai, D.57; Luo, B.13; Luo, T.1; Ma, B.10; Mahmoodifar, S.; Marisaldi, M.32; Martindale, A.8; Meidinger, N.15; Men, Y. P.8; Michalska, M.26; Mignani, R.34,35; Minuti, M.36; Motta, S.49; Muleri, F.2,58; Neilsen, J.51; Orlandini, M.32; Pan, A. T.56; Patruno, A.22,23; Perinati, E.3; Picciotto, A.8; Piemonte, C.8; Pinchera, M.36; Rachevski, A.43; Rapisarda, M.2,58; Rea, N.6,20; Rossi, E. M. R.22; Rubini, A.2,58; Sala, G.6; Shu, X. W.39; Sgro, C.36; Shen, Z. X.10; Soffitta, P.2; Song, L. M.1; Spandre, G.36; Stratta, G.50; Strohmayer, T. E.; Sun, L.1; Svoboda, J.44; Tagliaferri, G.24; Tenzer, C.3; Tong, H.30; Taverna, R.33; Torok, G.46; Turolla, R.8,33; Vacchi, A.43; Wang, J.1; Wang, J. X.39; Walton, D.8; Wang, K.10; Wang, J. F.55; Wang, R. J.1; Wang, Y. F.56; Weng, S. S.53; Wilms, J.25; Winter, B.8; Wu, X.7; Wu, X. F.8; Xiong, S. L.1; Xu, Y. P.1; Xue, Y. Q.39; Yan, Z.12; Yang, S.1; Yang, X.11; Yang, Y. J.1; Yuan, F.12; Yuan, W. M.11; Yuan, Y. F.39; Zampa, G.43; Zampa, N.43; Zdziarski, A.27; Zhang, C.11; Zhang, C. L.1; Zhang, L.56; Zhang, X.13; Zhang, Z.10; Zhang, W. D.12; Zheng, S. J.1; Zhou, P.13; Zhou, X. L.11
Conference NameSpace Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Source PublicationSpace Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Conference DateJune 26, 2016 - July 1, 2016
Conference PlaceEdinburgh, United kingdom
CountryUnited kingdom
Author of SourceThe Society of Photo-Optical Instrumentation Engineers (SPIE) Publisher: SPIE
Contribution Rank30
AbstractEXTP is a science mission designed to study the state of matter under extreme conditions of density, gravity and magnetism. Primary goals are the determination of the equation of state of matter at supra-nuclear density, the measurement of QED effects in highly magnetized star, and the study of accretion in the strong-field regime of gravity. Primary targets include isolated and binary neutron stars, strong magnetic field systems like magnetars, and stellar-mass and supermassive black holes. The mission carries a unique and unprecedented suite of state-of-the-art scientific instruments enabling for the first time ever the simultaneous spectral-timing-polarimetry studies of cosmic sources in the energy range from 0.5-30 keV (and beyond). Key elements of the payload are: the Spectroscopic Focusing Array (SFA) - a set of 11 X-ray optics for a total effective area of 0.9 m2and 0.6 m2at 2 keV and 6 keV respectively, equipped with Silicon Drift Detectors offering 180 eV spectral resolution; the Large Area Detector (LAD) - a deployable set of 640 Silicon Drift Detectors, for a total effective area of 3.4 m2, between 6 and 10 keV, and spectral resolution better than 250 eV; the Polarimetry Focusing Array (PFA) - a set of 2 X-ray telescope, for a total effective area of 250 cm2at 2 keV, equipped with imaging gas pixel photoelectric polarimeters; the Wide Field Monitor (WFM) - a set of 3 coded mask wide field units, equipped with position-sensitive Silicon Drift Detectors, each covering a 90 degrees 90 degrees field of view. The eXTP international consortium includes major institutions of the Chinese Academy of Sciences and Universities in China, as well as major institutions in several European countries and the United States. The predecessor of eXTP, the XTP mission concept, has been selected and funded as one of the so-called background missions in the Strategic Priority Space Science Program of the Chinese Academy of Sciences since 2011. The strong European participation has significantly enhanced the scientific capabilities of eXTP. The planned launch date of the mission is earlier than 2025. 2016 SPIE.
KeywordGamma rays Cosmology Ellipsometry Equations of state Gravitation Magnetism Polarimeters Silicon Silicon detectors Societies and institutions Space telescopes Spectral resolution Spectroscopy Stars Timing circuits
Indexed ByEI
EI Accession Number20165003128079
Citation statistics
Cited Times:98[WOS]   [WOS Record]     [Related Records in WOS]
Document Type会议论文
Affiliation1.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sc iences, Beijing 100049, China;
2.IAPS-INAF, Via del Fosso del Cavaliere 100 - 00133 Rome, Italy;
3.IAAT University of Tuebingen, Sand 1 - 72076 Tuebingen, Germany;
4.ISDC, Geneve University, Chemin d'Ecogia 16 - 1290 Versoix, Switzerland;
5.National Space Institute, Technical University of Denmark, Elektrovej Bld 327, 2800 Kgs Lyngby, Denmark;
6.Institute of Space Sciences (IEECCSIC), Campus UAB, C/Magrans s/n, Barcelona, Spain;
7.DPNC, Geneve University, Quai Ernest- Ansermet 30 - 1205 Geneva, Switzerland;
8.Department of Engineering Physics and Center for Astrophysics, Tsinghua University, Beijing 100084, China;
9.Key Laboratory of Advanced Microstructured Materials, Ministry of Education, Institute of Precision Optical Engineering, School of Physics Science and Engineering, Tongji University, Shanghai, 200090, China;
10.National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, China;
11.Shanghai Astronomical Observatory, 80 Nandan Road, Shanghai 200030, China;
12.Nanjing University, 22 Hankou Road Nanjing Jiangsu 210093, China;
13.Purdue University, 525 Northwestern Avenue, West Lafayette, IN 47907, United States;
14.Max Planck Institute for extraterrestrial Physics, Giessenbachstr. 1, Garching, Germany;
15.Peking University, No.5 Yiheyuan Road Haidian District, 100871, Beijing, China;
16.Center for Field Theory and Particle Physics and Department of Physics, Fudan University, 200433 Shanghai, China;
17.GXU-NAOC Center for Astrophysics and Space Sciences, Department of Physics, Guangxi University, Nanning 530004, China;
18.INAF-OA Roma, Via Frascati, 33 - 00040 Monte Porzio Catone, Italy;
19.Anton Pannekoek Institute, University of Amsterdam, Postbus 94249, Amsterdam, The Netherlands;
20.SRON, Sorbonnelaan 2 - 3584 CA Utrecht, The Netherlands;
21.Leiden Observatory, Niels Bohrweg 2 - NL- 2333 CA Leiden, The Netherlands;
22.ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA Dwingeloo, The Netherlands;
23.INAF - Brera Astronomical Observatory, via Bianchi 46, 23807, Merate (LC), Italy;
24.Remeis Observatory & ECAP, Universitaet Erlangen- Nuernberg, 96049 Bamberg, Germany;
25.Space Research Centre, Warsaw, Bartycka 18A - Warszawa, Poland;
26.Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18 PL-00-716 Warszawa, Poland;
27.Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada;
28.Department of Physics, Xiangtan University, Xiangtan 411105, China;
29.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, Xinjiang 830011, China;
30.Department of Astronomy, Beijing Normal University, Beijing 100875, China;
31.INAF-IASF Bologna, Via Gobetti 101, I- 40129 Bologna, Italy;
32.Department of Physics and Astronomy, University of Padova, via Marzolo 8, 35131 Padova, Italy;
33.INAF-IASF Milano, via E.Bassini 15, I-20133 Milano, Italy;(35Janusz Gil Institute of Astronomy, University of Zielona Góra, Lubuska 2, 65-265, Zielona Góra, Poland;
34.Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy;
35.Center for Data Science, New York University, 726 Broadway, 7th Floor, New York, NY 10003, USA;
36.University of Rome III, Via della Vasca Navale, 84 - 00146 Roma, Italy;
37.University of Science and Technology of China, No.96, JinZhai Road Baohe District, Hefei,Anhui, 230026, China;
38.CEA Saclay, DRF/IRFU, 91191 Gif sur Yvette, France;
39.University of Helsinki, Department of Physics, P.O.Box 48 FIN-00014 University of Helsinki, Finland;
40.Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Väisäläntie 20, FI-21500 Piikkiö, Finland;
41.Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Via A. Valerio 2 - I-34127, Trieste, Italy;
42.Astronomical Institute of the Academy of Sciences of the Czech Republic, Fricova 298, CZ-251 65 Ondrejov, Czech Republic;
43.Czech Technical University in Prague, Zikova 1903/4, CZ-166 36 Praha 6, Czech Republic;
44.Silesian University in Opava, Na Rybníčku 626/1 - 746 01 Opava, Czech Republic;
45.Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai 400005, India;
46.INAF-OA Capodimonte, Salita Moiariello, 16 - 80131 Napoli, Italy;
47.Oxford University, Department of Physics, Clarendon Laboratory, Parks Road, Oxford, OX1 3PU, United Kingdom;
48.Università degli Studi di Urbino Carlo Bo, Piazza della Repubblica 13, I-61029, Urbino, Italy;
49.MIT, 77 Massachusetts Avenue - MA 02139 Cambridge, United States;
50.Università dell’Insubria Via Valleggio 11, I-22100 Como, Italy;
51.Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing 210023, China;
52.Shanghai Institute of Satellite Engineering, ShangHai 200240, China;
53.Department of Astronomy and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen, Fujian 361005, China;
54.Institute of Spacecraft System Engineering, Beijing 100094, China;
55.Cornell Center for Astrophysics and Planetary Science, Department of Astronomy, Cornell University, Ithaca, NY 14853, USA;
56.INFN, Sez. Roma Tor Vergata, Via della Ricerca Scientifica 1 - 00133 Rome, Italy;
57.Fondazione Bruno Kessler, via Sommarive 18, I-38123 Povo (Trento), Italy;
58.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China;
59.University of Alabama in Huntsville, Huntsville, AL 35805, USA;
60.Astrophysics Science Division and Joint Space-Science Institute NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
Recommended Citation
GB/T 7714
Zhang, S. N.,Feroci, M.,Santangelo, A.,et al. EXTP: Enhanced X-ray Timing and Polarization mission[C]//The Society of Photo-Optical Instrumentation Engineers (SPIE) Publisher: SPIE:SPIE,2016:99051Q.
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