Fig. 12.
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Number counts of BHs from the simulations with Ṁrdw (left), ṀΓe (center), and ṀL/M (right). The shaded purple shows the result from single stellar evolution. The dashed pink, solid blue, and dash-dotted green lines show results from binary evolution of single BHs, binary BHs that do not merge within a Hubble time, and the resulting BH mass of a BBH merger that merged within a Hubble time, respectively.
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