eXTP: enhanced X-ray Timing and Polarimetry Mission

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

doi:https://dx.doi.org/10.1117/12.2232034

Number of the records: 1

eXTP: enhanced X-ray Timing and Polarimetry Mission

1.

SYSNO ASEP	0471269
Document Type	C - Proceedings Paper (int. conf.)
R&D Document Type	Conference Paper
Title	eXTP: enhanced X-ray Timing and Polarimetry Mission
Author(s)	Zhang, S.N. (CN) Feroci, M. (IT) Santangelo, A. (IT) Dong, Y.W. (CN) Feng, H. (CN) Lu, F.J. (CN) Nandra, K. (GB) Wang, Z.S. (CN) Zhang, S. (CN) Bozzo, E. (IT) Bursa, Michal (ASU-R)_{RID, ORCID} Dovčiak, Michal (ASU-R)_{RID, ORCID} Horák, Jiří (ASU-R)_{RID, ORCID} Hudec, René (ASU-R)_{RID, ORCID} Karas, Vladimír (ASU-R)_{RID, ORCID} Kunneriath, Devaky (ASU-R)_RID Svoboda, Jiří (ASU-R)_{RID, ORCID}
Number of authors	182
Source Title	Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray. - Bellingham : SPIE, 2016 - ISBN 9781510601895
Pages	99051q/1-99051q/16
Number of pages	16 s.
Publication form	Print - P
Action	Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Event date	26.06.2016 - 01.07.2016
VEvent location	Edinburgh
Country	GB - United Kingdom
Event type	WRD
Language	eng - English
Country	US - United States
Keywords	X-ray astronomy ; neutron Star EOS ; strong magnetism
Subject RIV	BH - Optics, Masers, Lasers
Institutional support	ASU-R - RVO:67985815
UT WOS	000387731500047
EID SCOPUS	85003530591
DOI	10.1117/12.2232034
Annotation	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).
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2017

Number of the records: 1