Large Observatory for x-ray Timing (LOFT-P): A Probe-class mission concept study

C.A. Wilson-Hodge, P.S. Ray, D. Chakrabarty, M. Feroci, L. Alvarez, M. Baysinger, C. Becker, E. Bozzo, S. Brandt, B. Carson, J. Chapman, A. Dominguez, L. Fabisinski, B. Gangl, J. Garcia, C. Griffith, M. Hernanz, R. Hickman, R. Hopkins, M. HuiL. Ingram, P. Jenke, Seppo Korpela, T. Maccarone, M. Michalska, M. Pohl, A. Santangelo, S. Schanne, A. Schnell, L. Stella, M. Van Der Klis, A. Watts, B. Winter, S. Zane, Takahashi T. Bautz M. (Redaktör), den Herder J.-W.A. (Redaktör)

Forskningsoutput: Kapitel i bok/rapport/konferenshandlingKonferensbidragVetenskapligPeer review


LOFT-P is a mission concept for a NASA Astrophysics Probe-Class (<$1B) X-ray timing mission, based on the LOFT M-class concept originally proposed to ESAs M3 and M4 calls. LOFT-P requires very large collecting area, high time resolution, good spectral resolution, broad-band spectral coverage (2-30 keV), highly flexible scheduling, and an ability to detect and respond promptly to time-critical targets of opportunity. It addresses science questions such as: What is the equation of state of ultra dense matter? What are the effects of strong gravity on matter spiraling into black holes? It would be optimized for sub-millisecond timing of bright Galactic X-ray sources including X-ray bursters, black hole binaries, and magnetars to study phenomena at the natural timescales of neutron star surfaces and black hole event horizons and to measure mass and spin of black holes. These measurements are synergistic to imaging and high-resolution spectroscopy instruments, addressing much smaller distance scales than are possible without very long baseline X-ray interferometry, and using complementary techniques to address the geometry and dynamics of emission regions. LOFT-P would have an effective area of >6 m2, > 10x that of the highly successful Rossi X-ray Timing Explorer (RXTE). A sky monitor (2-50 keV) acts as a trigger for pointed observations, providing high duty cycle, high time resolution monitoring of the X-ray sky with ∼20 times the sensitivity of the RXTE All-Sky Monitor, enabling multi-wavelength and multimessenger studies. A probe-class mission concept would employ lightweight collimator technology and large-area solid-state detectors, segmented into pixels or strips, technologies which have been recently greatly advanced during the ESA M3 Phase A study of LOFT. Given the large community interested in LOFT (>800 supporters∗, the scientific productivity of this mission is expected to be very high, similar to or greater than RXTE (∼ 2000 refereed publications). We describe the results of a study, recently completed by the MSFC Advanced Concepts Office, that demonstrates that such a mission is feasible within a NASA probe-class mission budget. © 2016 SPIE.
Titel på värdpublikationSpace Telescopes and Instrumentation 2016 : Ultraviolet to Gamma Ray
RedaktörerM. Bautz, T. Takahashi, J.-W.A. den Herder
ISBN (tryckt)9781510601895
StatusPublicerad - 2016
MoE-publikationstypA4 Artikel i en konferenspublikation
EvenemangSPIE Astronomical Telescopes + Instrumentation - Edinburgh, Storbritannien
Varaktighet: 26 juni 20161 juli 2016

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