Fig. B.2.
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Merger efficiency of compact binary objects per unit of stellar mass formed as a function of time and redshift in four different boxes of the MTNG simulations: MTNG46, MTNG92, MTNG185, and MTNG740 (from left to right). The total merger efficiency, along with the contributions from different merger channels, is displayed as indicated in the legend. Shaded regions represent constraints on the evolution of BBH merger efficiency at low redshifts (z ≲ 1), derived by extrapolating the (LVK25) limits as in Fig. 4.
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