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 oshaughnessy,R smith,E thrane,A vajpeyi· 0 min read URL Cite DOIpublicationLast updated on June 1, 2022 AuthorsB mckernanAuthorsK e s fordAuthorsT callisterAuthorsW m farrAuthorsR oshaughnessyAuthorsR smithAuthorsE thraneAuthorsA vajpeyi← A follow-up on intermediate-mass black hole candidates in the second LIGO–Virgo observing run with the Bayes Coherence Ratio August 1, 2022Deep follow-up of GW151226: ordinary binary or low-mass-ratio system? January 1, 2022 →