LISA: Parameter estimation for massive black hole binaries

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Gravitational Wave Detectors And Experiments, Gravitational Radiation Detectors, Mass Spectrometers, And Other Instrumentation And Techniques

Scientific paper

We calculate how accurately LISA and OMEGA can determine the parameters
of massive black hole binary systems by observing the signal emitted
during the in-spiral phase. In particular, we explore the role of the
black hole spins and the induced effect of precession of the source
orbital plane.

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