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Fig. 9.

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Effective spin correlations with relevant BBH parameters. The top row shows the probability density distribution for the primary BH mass, m1, and the effective spin, χeff, compared with posterior contour plots at credibility levels 50% and 90% of LVK BBH merger events GW190521 (dash-dotted red line, Abbott et al. 2020) and GW170729 (solid orange line, Abbott et al. 2023b), and LVK transient event GW190403_051519 (dashed yellow line, Abbott et al. 2021). The central (bottom) row has the same legend as the first row, but shows the mass ratio, q = m2/m1, (precession spin, χp) and the effective spin, χeff.

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