Parameter estimation for the GWTC-4.0 catalog with phenomenological waveform models that include orbital eccentricity and an updated description of spin precession
This paper extends the GWTC-4.0 catalog analysis of 84 binary black hole mergers by incorporating orbital eccentricity and an improved spin precession model into state-of-the-art IMRPhenom waveforms to provide updated posterior samples and quantify the impact of these effects on inferred source properties.