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eXTP: Enhanced X-ray Timing and Polarization mission

Shuang‐Nan ZhangM. FerociINAF - Istituto di Astrofisica e Planetologia Spaziali (Italy)A. SantangeloYongwei DongHua FengTsinghua Univ. (China)F. J. LuK. NandraMax-Planck-Institut für extraterrestrische Physik (Germany)Z. S. WangTongji Univ. (China)S. ZhangE. BozzoISDC Data Ctr. for Astrophysics (Switzerland)S. BrandtTechnical Univ. of Denmark (Denmark)Alessandra De RosaIAPS - INAF (Italy)Lijun GouNational Astronomical Observatories (China)M. HernanzInstitute of Space Sciences (Spain)M. van der KlisUniv. of Amsterdam (Netherlands)Xiang‐Dong LiInstitute of High Energy Physics (China)Yaqiang LiuP. OrleańskiSpace Research Ctr. (Poland)Giovanni PareschiINAF - Osservatorio Astronomico di Brera (Italy)M. PohlJuri PoutanenUniv. of Turku (Finland)Jin QuS. SchanneCEA-Ctr. de SACLAY (France)L. StellaINAF-OA Roma (Italy)P. UttleyUniv. of Amsterdam (Netherlands)Anna L. WattsUniv. of Amsterdam (Netherlands)Renxin XuPeking Univ. (China)Wenfei YuShanghai Astronomical Observatory (China)J. J. M. in ’t ZandSRON (Netherlands)Silvia ZaneMullard Space Science Lab. (United Kingdom)Laura ÁlvarezInstitute of Space Sciences (Spain)L. AmatiINAF - IASF Bologna (Italy)L. BaldiniIstituto Nazionale di Fisica Nucleare (Italy)Cosimo BambiFudan Univ. (China)Stefano BassoINAF - Osservatorio Astronomico di Brera (Italy)Sudip BhattacharyyaTata Institute of Fundamental Research (India)R. BellazziniIstituto Nazionale di Fisica Nucleare (Italy)T. BelloniINAF - Osservatorio Astronomico di Brera (Italy)P. BelluttiFondazione Bruno Kessler (Italy)S. BianchiUniv. degli Studi di Roma Tre (Italy)A. BrezIstituto Nazionale di Fisica Nucleare (Italy)Michal BursaAstronomical Institute of the ASCR, v.v.i. (Czech Republic)V. BurwitzMax-Planck-Institut für extraterrestrische Physik (Germany)C. Budtz-JørgensenDTU Space (Denmark)Ilaria CaiazzoUniv. of British Columbia (Canada)R. CampanaINAF - IASF Bologna (Italy)X. L. CaoP. CasellaINAF - Osservatorio Astronomico di Roma (Italy)C. Y. ChenShanghai Institute of Satellite Engineering (China)Li ChenShanghai Astronomical Observatory (China)Tianxiang ChenY. ChenInstitute of High Energy Physics (China)Y. ChenInstitute of High Energy Physics (China)Y. P. ChenInstitute of High Energy Physics (China)M. CivitaniINAF - Osservatorio Astronomico di Brera (Italy)F. Coti ZelatiUniv. of Amsterdam (Netherlands)Wei CuiInstitute of High Energy Physics (China)W. W. CuiInstitute of High Energy Physics (China)Z. G. DaiNanjing Univ. (China)E. Del MonteINAF - IASF Roma (Italy)D. de MartinoINAF - Osservatorio Astronomico di Capodimonte (Italy)Sergio Di CosimoINAF - IASF Roma (Italy)S. DieboldEberhard Karls Univ. Tübingen (Germany)Michal DovčiakAstronomical Institute of the Academy of Sciences of the Czech Republic (Czech Republic)I. DonnarummaINAF - IASF Roma (Italy)Victor DoroshenkoP. EspositoINAF-IASF Milano (Italy)Y. EvangelistaINAF - Istituto di Astrofisica e Planetologia Spaziali (Italy)Y. FavreP. FriedrichMax-Planck-Institut für extraterrestrische Physik (Germany)F. FuschinoINAF - IASF Bologna (Italy)J. L. GalvezInstitute of Space Sciences (Spain)Zeliang GaoInstitute of Spacecraft System Engineering (China)Mingyu GeO. GevinCommissariat à l'Énergie Atomique (France)D. GoetzCommissariat à l'Énergie Atomique (France)D. W. HanJeremy HeylUniv. of British Columbia (Canada)Jiří HorákAstronomical Institute of the Academy of Sciences of the Czech Republic (Czech Republic)W. HuFeifei HuangShanghai Institute of Optics and Fine Mechanics (China)Qunshan HuangInstitute of Precision Optical Engineering (China)R. HudecAstronomical Institute of the ASCR, v.v.i. (Czech Republic)D. HuppenkothenNew York Univ. (United States)G. L. IsraelINAF - Osservatorio Astronomico di Roma (Italy)A. IngramUniv. of Amsterdam (Netherlands)V. KarasAstronomical Institute of the ASCR, v.v.i. (Czech Republic)D. KarelinConsejo Superior de Investigaciones Científicas (Spain)Peter JenkeThe Univ. of Alabama in Huntsville (United States)L. JiS. KorpelaUniv. of Helsinki (Finland)D. KunneriathUniv. zu Köln (Germany)C. LabantiINAF - IASF Bologna (Italy)Gang LiXinxi LiInstitute of High Energy Physics (China)Li ChenXiangtan Univ. (China)E. W. LiangGuangxi Univ. (China)Olivier LimousinCEA-Ctr. de SACLAY (France)L. C.-C. LinBeijing Normal Univ. (China)Z. X. LingNational Astronomical Observatories (China)
2016en
ABI

Annotatsiya

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 &lt;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.

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