Fig. B.2.

Download original image
Spin hyperparameter posteriors of the COMPACTNESS PEAKS model, where μχ is the mean of the spin magnitude distribution, σχ is the width of the spin magnitude distribution, ζ is the fraction of BBHs in the subpopulation aligned with respect to the orbital angular momentum and σt is the width of the spin orientation distribution for the subpopulation aligned with respect to the orbital angular momentum for a given component. Left panel: The spin parameters paired with the BHL and BHH peaks Right panel: The spin parameters paired with the powerlaw (PL) component. The credible intervals on the 2D posterior distributions are at 1σ, 2σ and 3σ, using increasingly light shading. The intervals on the 1D posterior distributions are at 1σ.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.