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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 E3.

Marginal posteriors on the location μχ and scale σχ of the spin magnitude distribution within each mass bin under the CORRELATION model, along with the variance ﹩{ \mathcal V }﹩ of the log-likelihood estimator. Contours enclose the 50% and 90% credible regions.

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