Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 2.

The fraction ξ of sources in the Gaussian peak below ﹩\tilde{m}﹩ in the SUBPOPULATIONS model (blue), as well as ξ within each mass bin under the CORRELATION model.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse