Confusion noise level due to galactic and extragalactic binaries

Details Confusion noise level due to galactic and extragalactic binaries Confusion noise level due to galactic and extragalactic binaries

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cqgra..14.1439b&link_type=abstract

Classical and Quantum Gravity, Volume 14, Issue 6, pp. 1439-1444 (1997).

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We have revised our earlier rough estimate of the combined galactic and extragalactic binary confusion noise level curve for gravitational waves. This was done to correct some numerical errors and to allow for roughly three frequency bins worth of information about weaker sources being lost for each galactic binary signal that is removed from the data. The results are still based on the spectral amplitude estimates for different types of galactic binaries reported by Hils et al in 1990, and assume that the gravitational wave power spectral densities for other galaxies are proportional to the optical luminosities. The estimated confusion noise level drops to the LISA instrumental noise level at between roughly 3 and 8 mHz.

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