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 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, 2022Measuring the Properties of Active Galactic Nuclei Disks with Gravitational Waves May 1, 2022 →