Fig. 6.

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BH-BH total mass distribution within redshift 2 as a function of metallicity for M0 (top), M_αML1.82_MLTpp (middle), and M_αML1.5 (bottom). The dashed cyan line represents the metallicity threshold beyond which the formation of a convective envelope is estimated from the MESA tracks using MLT++ for M_αML1.82_MLTpp (see details in Sect. 3.6).
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