Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform?

@article{Cutler1994GravitationalWF,
  title={Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform?},
  author={Cutler and Flanagan},
  journal={Physical review. D, Particles and fields},
  year={1994},
  volume={49 6},
  pages={
          2658-2697
        }
}
  • Cutler, Flanagan
  • Published 1994
  • Physics, Medicine
  • Physical review. D, Particles and fields
The most promising source of gravitational waves for the planned kilometer-size laser-interferometer detectors LIGO and VIRGO are merging compact binaries, i.e., neutron-star\char21{}neutron-star (NS-NS), neutron-star\char21{}black-hole (NS-BH), and black-hole\char21{}black-hole (BH-BH) binaries. We investigate how accurately the distance to the source and the masses and spins of the two bodies will be measured from the inspiral gravitational wave signals by the three-detector LIGO-VIRGO… Expand
Parameter estimation on gravitational waves from neutron-star binaries with spinning components
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