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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 3 CONTRIBUTI IN ATTI DI CONVEGNO (Proceedings)
  4. 3.01 Contributi in Atti di convegno
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/26566
Title: eXTP: Enhanced X-ray Timing and Polarization mission
Authors: Zhang, S. N.
FEROCI, MARCO 
Santangelo, A.
Dong, Y. W.
Feng, H.
Lu, F. J.
Nandra, K.
Wang, Z. S.
Zhang, S.
Bozzo, E.
Brandt, S.
Liu, H. B.
Mahmoodifar, S.
Marisaldi, M.
DE ROSA, ALESSANDRA 
Martindale, A.
Meidinger, N.
Men, Y.
Michalska, M.
MIGNANI, Roberto 
Minuti, M.
Zhou X. L.
Motta, S.
MULERI, FABIO 
Neilsen, J.
ORLANDINI, MAURO 
Gou, L. J.
Pan, A. T.
Patruno, A.
Perinati, E.
Picciotto, A.
Piemonte, C.
Pohl, M.
Pinchera, M.
Rachevski A.
Rapisarda, M.
Rea, N.
Rossi, E. M. R.
Hernanz, M.
Rubini, A.
Sala, G.
Shu, X. W.
Sgro, C.
Poutanen, J.
Shen, Z. X.
SOFFITTA, PAOLO 
Song, L.
Spandre, G.
Stratta, G.
Strohmayer, T. E.
van der Klis, M.
Sun, L.
Svoboda, J.
TAGLIAFERRI, Gianpiero 
Qu, J. L.
Tenzer, G.
Hong, T.
Taverna, R.
Torok, G.
Turolla, R.
Vacchi, S.
Wang, J.
Li, X. D.
Walton, D.
Wang, K.
Schanne, S.
Wang, J. F.
Wang, R. J.
Wang, Y. F.
Weng, S. S.
Wilms, J.
Winter, B.
Wu, X.
Wu, X. F.
Liu, Y.
Xiong, S. L.
STELLA, Luigi 
Xu, Y. P.
Xue, Y. Q.
Yan, Z.
Yang, S.
Yang, X.
Yang, Y. J.
Yuan, F.
Yuan, W. M.
Yuan, Y. F.
Orleanski, P.
Uttley, P.
Zampa, G.
Zampa, N.
Zdziarski, A.
Zhang, C.
Zhang, C. L.
Zhang, L.
Zhang, X.
Zhang, Z.
Zhang, W. D.
Zheng, S. J.
Watts, A.
PARESCHI, Giovanni 
Zhou, P.
Xu, R. X.
Yu, W. F.
Liu, H. W.
in 't Zand, J. J. M.
Zane, S.
Alvarez, L.
AMATI, LORENZO 
Baldini, L.
Bambi, C.
BASSO, Stefano 
Bhattacharyya S.
Bellazzini, R.
BELLONI, Tomaso Maria Melchiorre 
Liu, Z.
Bellutti, P.
BIANCHI, SIMONE
Brez, A.
Bursa, M.
Burwitz, V.
Budtz-Jørgensen, C.
Caiazzo, I.
CAMPANA, RICCARDO 
Cao, X.
CASELLA, Piergiorgio 
Lu, B.
Chen, C. Y.
Chen, L.
Chen, T.
Chen, Y.
Chen, Y. P.
CIVITANI, Marta Maria 
Coti Zelati, F.
Cui, W.
Cui, W. W.
Dai, Z. G.
Lund, N.
DEL MONTE, Ettore 
DE MARTINO, Domitilla 
Di Cosimo, S.
Diebold, S.
Dovciak, M.
Donnarumma, I.
Doroshenko, V.
Esposito, P.
EVANGELISTA, YURI 
Favre, Y.
Lai, D.
Friedrich, P.
FUSCHINO, FABIO 
Galvez, J. L.
Gao, Z. L.
Ge, M. Y.
Gevin, O.
Goetz, D.
Han, D. W.
Heyl, J.
Horak, J.
Luo, B.
Hu, W.
Huang, F.
Huang, Q. S.
Hudec, R.
Huppenkothen, D.
ISRAEL, Gian Luca 
Ingram, A.
Karas, V.
Karelin, D.
Jenke, P. A.
Luo, T.
Ji, L.
Korpela, S.
Kunneriath, D.
LABANTI, CLAUDIO 
Li, G.
Li, X.
Li, Z. S.
Liang, E. W.
Limousin, O.
Lin, L.
Ma, B.
Ling, Z. X.
Issue Date: 2016
Volume: Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Editors: den Herder, Jan-Willem A.; Takahashi, Tadayuki; Bautz, Marshall
Series: PROCEEDINGS OF SPIE 
Number: 9905
First Page: 99051Q
Abstract: eXTP 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 m<SUP>2</SUP> and 0.6 m<SUP>2</SUP> at 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 m<SUP>2</SUP>, 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 cm<SUP>2</SUP> at 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 x 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.
Conference Name: Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Conference Place: Edinburgh, United Kingdom
Conference Date: 26 June - 1 July 2016
URI: http://hdl.handle.net/20.500.12386/26566
URL: http://arxiv.org/abs/1607.08823v1
https://www.spiedigitallibrary.org/conference-proceedings-of-spie/9905/1/eXTP-Enhanced-X-ray-Timing-and-Polarization-mission/10.1117/12.2232034.full
ISSN: 0277-786X
ISBN: 9781510601901
9781510601895
DOI: 10.1117/12.2232034
Bibcode ADS: 2016SPIE.9905E..1QZ
Fulltext: open
Appears in Collections:3.01 Contributi in Atti di convegno

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