Parameter estimation for inspiraling eccentric compact binaries including pericenter precession

@article{Mikoczi2012ParameterEF,
  title={Parameter estimation for inspiraling eccentric compact binaries including pericenter precession},
  author={Bal'azs Mik'oczi and Bence Kocsis and P'eter Forg'acs and M'aty'as Vas'uth},
  journal={Physical Review D},
  year={2012},
  volume={86},
  pages={104027}
}
Inspiraling supermassive black hole binary systems with high orbital eccentricity are important sources for space-based gravitational wave (GW) observatories like the Laser Interferometer Space Antenna (LISA). Eccentricity adds orbital harmonics to the Fourier transform of the GW signal and relativistic pericenter precession leads to a three-way splitting of each harmonic peak. We study the parameter estimation accuracy for such waveforms with different initial eccentricity using the Fisher… 
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