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Stellar-mass Black Hole Parameter Estimation Achieves Improved Accuracy With Center-of-Mass Acceleration
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Stellar-mass Black Hole Parameter Estimation Achieves Improved Accuracy With Center-of-Mass Acceleration
Future gravitational wave detectors will be able to discern the subtle influence of distant, massive objects on merging black holes, allowing scientists to measure these effects with unprecedented precision and avoid significant errors in determining the properties of the merging pair.
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