Sharper Lenses on Gravitational Waves: A New Bayesian Twist

A breakthrough method uses each waveform model’s known accuracy to guide a single Bayesian analysis, prioritizing the sharpest tool for every part of the parameter space. The result is faster, less biased inferences that better reveal black-hole properties. In tests and for GW19910717, it tightens mass estimates, confirms unequal masses, and strengthens evidence for hierarchical formation.

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