An extended phenomenological template for core-bounce GW signals recovers the rotational parameter β with a median relative error of 11.93% when analyzed via MCMC in real O3aL1 noise.
Black holes, white dwarfs and neutron stars: the physics of compact objects
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Bayesian parameter estimation for the Core-bounce phase of Rapidly Rotating Core-Collapse Supernovae in real interferometric data
An extended phenomenological template for core-bounce GW signals recovers the rotational parameter β with a median relative error of 11.93% when analyzed via MCMC in real O3aL1 noise.