STUCHLÍK, Zdeněk, Gabriel TÖRÖK and M. FEROCI. The Large Observatory for X-ray Timing (LOFT). Experimental Astronomy. NL - Nizozemsko, 2012, vol. 34, No 2, p. 415-444. ISSN 0922-6435. Available from: https://dx.doi.org/10.1007/s10686-011-9237-2.
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Basic information
Original name The Large Observatory for X-ray Timing (LOFT)
Authors STUCHLÍK, Zdeněk, Gabriel TÖRÖK and M. FEROCI.
Edition Experimental Astronomy, NL - Nizozemsko, 2012, 0922-6435.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
WWW URL
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1007/s10686-011-9237-2
UT WoS 000309230600010
Keywords in English Missions; X-ray timing; Compact objects; Black holes; Neutron stars
Tags
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 7/4/2021 07:58.
Abstract
High-time-resolution X-ray observations of compact objects provide direct access to strong-field gravity, to the equation of state of ultradense matter and to black hole masses and spins. A 10 m(2)-class instrument in combination with good spectral resolution is required to exploit the relevant diagnostics and answer two of the fundamental questions of the European Space Agency (ESA) Cosmic Vision Theme "Matter under extreme conditions", namely: does matter orbiting close to the event horizon follow thepredictions of general relativity? What is the equation of state of matter in neutron stars? The Large Observatory For X-ray Timing (LOFT), selected by ESA as one of the four Cosmic Vision M3 candidate missions to undergo an assessment phase, will revolutionise the study of collapsed objects in our galaxy and of the brightest supermassive black holes in active galactic nuclei. Thanks to an innovative design and the development of large-area monolithic silicon drift detectors, the Large
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