Magnetar population data show no statistical requirement for a distinct white-dwarf channel; a single neutron-star model suffices.
year 2024
2 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 2representative citing papers
GP15 maps BBH spectrograms to parameter posteriors via residual networks and normalizing flows, producing results consistent with LVK analyses on GWTC-2.1 and GWTC-3 events while running in seconds.
citing papers explorer
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Data-Driven Constraints on Magnetar Population: No Evidence for a Distinct White Dwarf Channel
Magnetar population data show no statistical requirement for a distinct white-dwarf channel; a single neutron-star model suffices.
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Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data
GP15 maps BBH spectrograms to parameter posteriors via residual networks and normalizing flows, producing results consistent with LVK analyses on GWTC-2.1 and GWTC-3 events while running in seconds.