Annual modulation of the Galactic binary confusion noise bakground and LISA data analysis

Details Annual modulation of the Galactic binary confusion noise bakground and LISA data analysis Annual modulation of the Galactic binary confusion noise bakground and LISA data analysis

2004-03-02

arxiv.org/abs/gr-qc/0403014v1

Phys.Rev. D69 (2004) 123005

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, 6 figures

Scientific paper

10.1103/PhysRevD.69.123005

We study the anisotropies of the Galactic confusion noise background and its effects on LISA data analysis. LISA has two data streams of the gravitational waves signals relevant for low frequency regime. Due to the anisotropies of the background, the matrix for their confusion noises has off-diagonal components and depends strongly on the orientation of the detector plane. We find that the sky-averaged confusion noise level $\sqrt {S(f)}$ could change by a factor of 2 in three months, and would be minimum when the orbital position of LISA is either around the spring or autumn equinox.

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