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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 D2.

Simulated effective spin χeff distribution used for mock catalog realizations (black) compared to effective spin PPDs recovered by two LVK analyses: the PPD implied by the B-spline analysis (blue), and the marginal PPD when directly modeling the population distribution of χeff and effective precessing spin χp as a bivariate Gaussian (orange; A. G. Abac et al. 2026b). Medians are denoted with solid lines and shaded regions enclose the 90% credible region.

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