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Parameter estimation for Galactic binaries by LISA

Ryuichi Takahashi·Naoki Seto
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Abstract

We calculate how accurately parameters of the short-period binaries $(10^{-4} {Hz} \lsim f\lsim 10^{-2} {Hz})$ will be determined from the gravitational waves by LISA. In our analysis the chirp signal ${\dot f}$ is newly included as a fitting parameters and dependence on observational period or wave frequency is studied in detail. Implications for gravitational wave astronomy are also discussed quantitatively.

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Ryuichi Takahashi, Naoki Seto. 2002-04-29. Parameter estimation for Galactic binaries by LISA. https://doi.org/10.1086/341483

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