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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 E4.

Marginal posteriors on the parameters of the primary mass, mass ratio, and redshift population distributions obtained under the SUBPOPULATIONS model (blue, filled regions) as well as the CORRELATION model (purple lines). See Table 2 for parameter definitions and priors. We also show the variance ﹩{ \mathcal V }﹩ of the log-likelihood estimator. Contours enclose the 50% and 90% credible regions.

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