Semi-agnostic Equation of State models for Bayesian inference with Neutron Star observations
Semi-agnostic Equation of State models for Bayesian inference with Neutron Star observations
Poster 280: Nolan Davis on comparisons of waveform approximants for GW signals
Poster 280: Nolan Davis on comparisons of waveform approximants for GW signals
Poster 215: Lyla Traylor on building our prior distribution for the high-density neutron star equation of state
Poster 215: Lyla Traylor on building our prior distribution for the high-density neutron star equation of state
- Emily Wuchner will be discussing measurements of neutron-star tidal parameters at Tuesday at 11:09 Session H20
- Ryan Johnson showing how he can correct for waveform uncertainty in compact binary inference on Tuesday at 2:54 in Session J17.
- Emily Wuchner will be discussing measurements of neutron-star tidal parameters at Tuesday at 11:09 Session H20
- Ryan Johnson showing how he can correct for waveform uncertainty in compact binary inference on Tuesday at 2:54 in Session J17.