P. J. Easter
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View article: Bilby: A User-friendly Bayesian Inference Library for Gravitational-wave Astronomy
Bilby: A User-friendly Bayesian Inference Library for Gravitational-wave Astronomy Open
Bayesian parameter estimation is fast becoming the language of gravitational-wave astronomy. It is the method by which gravitational-wave data is used to infer the sources' astrophysical properties. We introduce a user-friendly Bayesian in…
View article: Can we measure the collapse time of a post-merger remnant for a future GW170817-like event?
Can we measure the collapse time of a post-merger remnant for a future GW170817-like event? Open
Measuring the collapse time of a binary neutron star merger remnant can inform the physics of extreme matter and improve modelling of short gamma-ray bursts and associated kilonova. The lifetime of the post-merger remnant directly impacts …
View article: Detection and parameter estimation of binary neutron star merger remnants
Detection and parameter estimation of binary neutron star merger remnants Open
Detection and parameter estimation of binary neutron star merger remnants can\nshed light on the physics of hot matter at supranuclear densities. Here we\ndevelop a fast, simple model that can generate gravitational waveforms, and\nshow it…
View article: Computing fast and reliable gravitational waveforms of binary neutron star merger remnants
Computing fast and reliable gravitational waveforms of binary neutron star merger remnants Open
Gravitational waves have been detected from the inspiral of a binary\nneutron-star, GW170817, which allowed constraints to be placed on the neutron\nstar equation of state. The equation of state can be further constrained if\ngravitational…