An HHT-based pipeline estimates protoneutron star mass/radius-squared from simulated core-collapse supernova gravitational waves with accuracy comparable to STFT-based methods.
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Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform
An HHT-based pipeline estimates protoneutron star mass/radius-squared from simulated core-collapse supernova gravitational waves with accuracy comparable to STFT-based methods.