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Table 1.

Parameters and settings of our model.

Parameter Description Prior/Value
Mh, seed [M] Minimum mass of the halos that host a seed BH log𝒰[106, 107.7]
fseed Probability to seed a leaf halo with Mh ≥ Mh, seed at z ≥ 10 log𝒰[0.01, 1]
μseed [M] Mean of the log-normal distribution of seed masses log𝒰[102.5, 106]
σseed [dex] Standard deviation of the log-normal distribution of seed masses log𝒰[100.5, 102]
tdelay [Myr] Additional time delay (after DF timescale) for BH binary merger log𝒰[10−0.5, 104]
tburst [Myr] Duration of burst accretion mode log𝒰[1, 100]
γburst Slope of the power-law distribution of fEdd, burst 𝒰[−1, 0]
μsteady [dex] Mean of the log-normal distribution of fEdd, steady 𝒰[−6, −3]
σsteady [dex] Standard deviation of the log-normal distribution of fEdd, steady 𝒰[0.5, 3]
zcut Redshift below which accretion is cut in the most massive BHs 𝒰[1, 4]
mcut, 0 [M] Mass at z = 0 above which accretion is cut log𝒰[106, 107.3]
αcut Slope of the increase in the mass cut for accretion with redshift, see Eq. (8) 𝒰[0, 0.5]

fEdd, burst Burst mode Eddington ratio 𝒫ℒ(γburst − 1, 10−2, 10)
fEdd, steady Steady mode Eddington ratio log𝒩(μsteady, σsteady)≤1
tsteady [Myr] Duration of a steady accretion episode, after which fEdd, steady, tsteady are redrawn log𝒰[1, 100]
ϵ Radiative efficiency 0.1
qh, major Mass ratio threshold for major halo mergers 0.13
pmulti Probability of interaction between three or more BHs 0.22

Notes. The first 12 lines (before the double bar) list the free parameters of our model, which we fit to observations. The remaining lines summarise the distributions on quantities entering the simulations and the parameters that are fixed in our model. In the third column, (log) 𝒰 stands for a (log-) uniform distribution in the given range, 𝒫ℒ for a power-law distribution with given slope and range and log𝒩 for a log-normal distribution with given mean and standard deviation.

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