LIGO–Virgo correlations between mass ratio and effective inspiral spin: testing the active galactic nuclei channelJune 1, 2022·B McKernan,K E S Ford,T Callister,W M Farr,R O’Shaughnessy,R Smith,E Thrane,A Vajpeyi· 0 min read URL Cite DOIpublicationLast updated on June 1, 2022 ← A follow-up on intermediate-mass black hole candidates in the second LIGO–Virgo observing run with the Bayes Coherence Ratio August 1, 2022Bayesian inference for compact binary coalescences with <scp>bilby</scp>: validation and application to the first LIGO–Virgo gravitational-wave transient catalogue September 1, 2020 →