Deep follow-up of GW151226: ordinary binary or low-mass-ratio system?January 1, 2022·Avi vajpeyi,Avi vajpeyi,Rory smith,Eric thrane· 0 min read CitepublicationLast updated on January 1, 2022 AuthorsAvi vajpeyiAuthorsAvi vajpeyiAuthorsRory smithAuthorsEric thrane← LIGO–Virgo correlations between mass ratio and effective inspiral spin: testing the active galactic nuclei channel June 1, 2022A search for intermediate-mass black holes mergers in the second LIGO--Virgo observing run with the Bayes Coherence Ratio January 1, 2021 →