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eXTP: Enhanced X-ray Timing and Polarization mission
Zhang SN(张双南); Dong YW(董永伟); Lu FJ(卢方军); Zhang S(张澍); Liu Y(刘元); Qu JL(屈进禄); Cao XL(曹学蕾); Chen TX(陈田祥); Chen Y(陈勇); Chen YP(陈玉鹏); Cui WW(崔苇苇); Han DW(韩大炜); Hu W(胡渭); Li G(李刚); Li X(李鲜); Liu HW(刘华微); Lu B(陆波); Luo T(雒涛); Song LM(宋黎明); Sun L(孙亮); Wang J(王娟); Wang RJ(王瑞杰); Xiong SL(熊少林); XU XP; Yang S(杨生); Yang YJ(杨彦佶); Zhang CL(张春雷); Zheng SJ(郑世界)
2016
Source PublicationSPIE Proceedings
ISSN0277-786X
EISSN1996-756X
ISBN978-1-5106-0189-5; 978-1-5106-0190-1
Issue9905Pages:99051Q
Corresponding Author张双南
SubtypeProceedings Paper
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 similar to 0.9 m(2) and 0.6 m(2) 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 similar to 3.4 m(2), 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(2) 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 TitleConference on Space Telescopes and Instrumentation - Ultraviolet to Gamma Ray
Conference PlaceEdinburgh, SCOTLAND
Conference DateJUN 26-JUL 01, 2016
KeywordX-ray astronomy Neutron Star EOS Strong Magnetism Strong Gravity X-ray timing spectroscopy
DOI10.1117/12.2232034
Indexed ByCPCI ; ADS ; ADS
Language英语
WOS IDWOS:000387731500047
ADS Bibcode2016SPIE.9905E..1QZ
ADS URLhttps://ui.adsabs.harvard.edu/abs/2016SPIE.9905E..1QZ
ADS CITATIONShttps://ui.adsabs.harvard.edu/abs/2016SPIE.9905E..1QZ/citations
inspireid1478578
Citation statistics
Cited Times:80 [INSPIRE]
Cited Times:134 [ADS]
Document Type期刊论文
Identifierhttp://ir.ihep.ac.cn/handle/311005/260846
Collection粒子天体物理中心
Affiliation中国科学院高能物理研究所
Recommended Citation
GB/T 7714
Zhang SN,Dong YW,Lu FJ,et al. eXTP: Enhanced X-ray Timing and Polarization mission[J]. SPIE Proceedings,2016(9905):99051Q.
APA 张双南.,董永伟.,卢方军.,张澍.,刘元.,...&郑世界.(2016).eXTP: Enhanced X-ray Timing and Polarization mission.SPIE Proceedings(9905),99051Q.
MLA 张双南,et al."eXTP: Enhanced X-ray Timing and Polarization mission".SPIE Proceedings .9905(2016):99051Q.
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