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Fig. 7

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Merger times and galaxy present-day stellar masses of the BBH mergers in FIREbox estimated from the ‘Gamma’ cluster formation model (colormap). The left and top subplots show the marginalised distributions obtained with the three different models of cluster formation (coloured lines), as well as the corresponding distributions for all star formation in the 979 galaxies identified inside FIREbox (black solid line, with arbitrary normalisation).

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