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The origin and formation of stellar-mass binary black holes remains an open question that can be addressed by precise measurements of the binary and orbital parameters from their gravitational-wave signal.
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Thibault Damour, Piotr Jaranowski, and Gerhard Schaefer, “On the determination of the last stable orbit for circular general relativistic binaries at the third postNewtonian approximation,” Phys. Rev. D62
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Johan Samsing, “Eccentric Black Hole Mergers Forming in Globular Clusters,” Phys. Rev. D97
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