Modeling the remnant mass, spin, and recoil from unequal-mass, precessing black-hole binaries: The intermediate mass ratio regime
Published in Physical Review D 92, 024022
(Monday, July 13, 2015)
Abstract
he fits presented in the paper had an error in Lisco and were also not optimized for the aligned spin case. Of these two, the latter has a larger effect when using the formula for extrapolation. In addition, there were errors in the remnant spins obtained from the radiated angular momentum in Table XVIII.
