Exploration of features in the black hole mass spectrum inspired by non-parametric analyses of gravitational wave observations

Open Access

Fig. 4.

Left: Marginal posterior distribution for λ for the EVOLVING model conditioned on κ_PL = κ_Peak and for the POWERLAW+PEAK model. Right: Marginal posterior distribution for the redshift spectral index κ for the PowerLaw, Peak, and POWERLAW+PEAK population model.

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.