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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 E1.

Inset figures from Figure 1 showing priors and posteriors on the marginal density of the population-level spin tilt distribution averaged over a window of ±0.1 around ﹩\cos \tau =0﹩ under the SUBPOPULATIONS (left) and CORRELATION (right) models. Colors and line styles match Figure 1.

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