Harmonic Correlation For Eccentric Binaries In Lisa Gravitational Wave Observations

Details Harmonic Correlation For Eccentric Binaries In Lisa Gravitational Wave Observations Harmonic Correlation For Eccentric Binaries In Lisa Gravitational Wave Observations

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21344902l&link_type=abstract

American Astronomical Society, AAS Meeting #213, #449.02; Bulletin of the American Astronomical Society, Vol. 41, p.340

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Binary systems will be among the most numerous sources detected by interferometric gravitational wave detectors, such as LISA. In many instances, the binaries will have non-zero orbital eccentricities, producing power in the Fourier spectrum at the fundamental orbital frequency and its higher harmonics. This talk describes a binary search technique called harmonic correlation which exploits the harmonic structure of the signal to identify binaries in gravitational wave data streams, even at low signal-to-noise ratios. The analysis procedure is outlined, and demonstrated on realistic simulated LISA data streams.

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