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Fig. 2.

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Joint posterior distributions of the parameters describing the binary progenitors of 3C 186. We show one- and two-dimensional marginal posteriors for the mass ratio (q), spin magnitudes (χ1, 2), spin inclination angles (θ1, 2), the in-plane azimuthal angle of the heavier BH spin (ϕ1), the difference between the azimuthal angles (Δϕ), polar observation angles (θn), and the azimuthal observation angle (ϕn). Contours indicate 90% and 50% credible regions.

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