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Fig. 5.

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Posterior on the model parameters related to seeding and BH mergers when fitting for the LF and GW background. We show the mean and standard deviation of the log-normal distribution of seed BH masses, μseed and σseed; the minimum mass of haloes seeded Mh, seed and the seeding probability fseed; the delay of binary BH mergers (in addition to halo dynamical friction), tdelay.

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