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Secondary-mass Features Improve Spectral-siren H0 Constraints
Yin-Jie Li et al 2026 The Astrophysical Journal 1010 .
Caption: Figure 3.
Mass distribution of primary and secondary BHs. The solid lines and shaded areas are for median values and 90% credible intervals.
© 2026. The Author(s). Published by the American Astronomical Society.
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