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Compact binaries inspiralling along quasi-circular orbits are the most plausible gravitational wave (GW) sources for the operational, planned and proposed laser interferometers.
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T. Damour and G. Schäfer, Nuovo Cimento Soc. Ital. Fis., B 101
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T. Damour and N. Deruelle, Ann. Inst. Henri Poincare Phys. Theor. 43
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T. Damour, A. Gopakumar, and B. R. Iyer, Phys. Rev. D 70
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T. Damour and N. Deruelle, Ann. Inst. Henri Poincaré Phys. Théor. 44
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T. Damour, P. Jaranowski, and G. Schäfer, Phys. Lett. B 513
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Cited in the paper.
C. Königsdörffer and A. Gopakumar, Phys. Rev. D 73
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M. Tessmer and A. Gopakumar, submitted to Phys. Rev. D (2007), arXiv:0712.3199[gr-qc]
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M. Tessmer and A. Gopakumar, Mon. Not. Roy. Astron. Soc. 374
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