Fig. 9.
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Chirp mass (M1M2)3/5(M1 + M2)−1/5 distribution of IMBH mergers in the L12.5 simulations to z = 5. While the precise normalisation is somewhat arbitrary, the differences due to different accretion rate estimates is significant, with the tng and mod ff models being dominated by seed-mass mergers, while ff is far more distributed due to growth via accretion.
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