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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 B1.

PPDs on the marginal density of sources as a function of spin tilt ﹩\cos \tau ﹩ (left) and magnitude χ (right) in four bins of BH mass under the CORRELATION model, using a different choice of bin edges than the results presented in Section 3.

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