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No Model-independent Evidence for a Peak in Binary Black Hole Spin (Mis)alignments

  • Authors: Noah E. Wolfe, Salvatore Vitale, Michael Zevin

Noah E. Wolfe et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure C1.

Joint marginal posterior on the branching ratio ξ between low-mass isotropic and Gaussian spin tilt distributions under the SUBPOPULATIONS model, as well as the location (μχ, ﹩{\mu }_{\chi }^{\,{\rm{Iso}}\,}﹩, and ﹩{\sigma }_{\chi }^{\,{\rm{High\, Iso}}\,}﹩) and scale (σχ, ﹩{\sigma }_{\chi }^{\,{\rm{Iso}}\,}﹩, and ﹩{\sigma }_{\chi }^{\,{\rm{High\, Iso}}\,}﹩) parameters of the spin distributions for each respective subpopulation. Contours shown enclose the 50% and 90% credible regions.

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