Combining BAYESTACK radius posteriors for four masses through a common piecewise-polytrope EoS forecasts ~1 km (uniform prior) or ~0.55 km (astrophysical prior) radius constraints from A+ era post-merger signals.
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Prospect of Constraining the EoS of Neutron Stars Using Post-Merger Signals
Combining BAYESTACK radius posteriors for four masses through a common piecewise-polytrope EoS forecasts ~1 km (uniform prior) or ~0.55 km (astrophysical prior) radius constraints from A+ era post-merger signals.