HomeResearchRelativistic Compact ObjectsGravitational Waveform ModelingObservation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks.

Observation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks.

Dependence of SNR change due to eccentricity for Cosmic Explorer.

Change in sensitivity for Cosmic Explorer for a 50-10 solar masses system optimally oriented.

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