Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Secondary-mass Features Improve Spectral-siren H0 Constraints

  • Authors: Yin-Jie Li, Yi-Ying Wang, Yuan-Zhu Wang, Shao-Peng Tang, Yi-Zhong Fan

Yin-Jie Li et al 2026 The Astrophysical Journal 1010 .

  • Provider: AAS Journals

Caption: Figure B4.

Posterior distributions of the Hubble constant and the parameters describing the BBH mass distribution for the Flexible-BBH, PS-paired, MLTP-paired, and MLTP models. The four peaks correspond to the maxima of the cubic spline functions for the Flexible-BBH and PS-paired models, as illustrated in Appendix C.1.

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
Copyright and Terms & Conditions

Additional terms of reuse