Large Observatory for x-ray Timing (LOFT-P): A Probe-classs Mission Concept Study
Colleen A. Wilson-Hodge, Paul S. Ray, Deepto Chakrabarty, Marco, Feroci, Laura Alvarez, Michael Baysinger, Chris Becker, Enrico Bozzo, Soren, Brandt, Billy Carson, Jack Chapman, Alexandra Dominguez, Leo Fabisinski, Bert, Gangl, Jay Garcia, Christopher Griffith, Margarita Hernanz

TL;DR
LOFT-P is a proposed NASA X-ray timing mission with a large collecting area, high time resolution, and broad spectral coverage, designed to study extreme astrophysical phenomena like neutron stars and black holes.
Contribution
This study presents a feasible concept for LOFT-P, a probe-class mission with advanced X-ray timing capabilities, within NASA's budget constraints.
Findings
LOFT-P can achieve >6 m^2 collecting area, >10x RXTE sensitivity.
The mission enables sub-millisecond timing studies of neutron stars and black holes.
Feasibility demonstrated within NASA probe-class budget.
Abstract
LOFT-P is a concept for a NASA Astrophysics Probe-Class (<$1B) X-ray timing mission, based on the LOFT concept originally proposed to ESAs M3 and M4 calls. LOFT-P requires very large collecting area (>6 m^2, >10x RXTE), 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 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…
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