eXTP: enhanced X-ray Timing and Polarimetry Mission

0471269 - ASÚ 2017 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
Zhang, S.N. - Feroci, M. - Santangelo, A. - Dong, Y.W. - Feng, H. - Lu, F.J. - Nandra, K. - Wang, Z.S. - Zhang, S. - Bozzo, E. - Bursa, Michal - Dovčiak, Michal - Horák, Jiří - Hudec, René - Karas, Vladimír - Kunneriath, Devaky - Svoboda, Jiří … celkem 182 autorů
eXTP: enhanced X-ray Timing and Polarimetry Mission.
Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray. Bellingham: SPIE, 2016, 99051Q/1-99051Q/16. Proceedings of SPIE, 9905. ISBN 9781510601895.
[Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray. Edinburgh (GB), 26.06.2016-01.07.2016]
Institucionální podpora: RVO:67985815
Klíčová slova: X-ray astronomy * neutron Star EOS * strong magnetism
Kód oboru RIV: BH - Optika, masery a lasery

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).
Trvalý link: http://hdl.handle.net/11104/0268665