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Accurate waveform models for coalescing binaries on eccentric orbits are crucial for avoiding biases in the analysis of eccentric gravitational-wave signals.
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J. Downing, M. Benacquista, M. Giersz, and R. Spurzem, Compact binaries in star clusters–i. black hole binaries inside globular clusters, Monthly Notices of the Royal Astronomical Society 407
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I. Mandel and A. Farmer, Merging stellar-mass binary black holes, Phys. Rept. 955
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