T. J. Maccarone, R. A. M. Wijnands, N. Degenaar, A. Archibald, A. Watts, S. Vaughan, G. Wynn, G. Knevitt, W. Farr, N. Andersson, M. van der Klis
Published 2015-01-12Version 1
This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of very faint X-ray binaries, orbital period distribution of black hole X-ray binaries and neutron star spin up. For a summary, we refer to the paper.
Comments: White Paper in Support of the Mission Concept of the Large Observatory for X-ray Timing
Explaining the 'outliers' track in Black Hole X-ray Binaries with the BZ-jet and inner-disk coupling
Revealing the Galactic Population of BHs
Hard state neutron star and black hole X-ray binaries in the radio:X-ray luminosity plane
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