July 20, 2015 by Davide Gerosa Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II: Full parameter estimation Daniele Trifirò, Richard O’Shaughnessy, Davide Gerosa, Emanuele Berti, Michael Kesden, Tyson Littenberg, Ulrich Sperhake. Physical Review D 93 (2016) 044071. arXiv:1507.05587 [gr-qc]. This is a follow up of arXiv:1403.7147, just done better. Instead of overlaps, we do real injections in LIGO parameter-estimation codes to show that spin-orbit resonances are indeed detectable.