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Table 1.

Characteristic parameters of our simulation runs.

ID Simulation inputs from SED fits Comments
β0 ρflr uflr a Risco HIGH−mass LOW−mass
SIM20 10 10−5 10−8 0.9375 2 Rg 2.0×10−5 5.6×10−7 reference run, similar to Vourellis et al. (2019)
SIM21 10 10−4 10−6 0.9375 2 Rg 1.0×10−5 5.0×10−7 as SIM20, floor density higher
SIM22 10 10−4 10−6 0.0 6 Rg 7.0×10−5 5.0×10−6 as SIM20, a = 0, infall to BH, disk wind
SIM23 10 10−3 10−5 0.9375 2 Rg 3.0×10−6 1.5×10−7 as SIM21, floor even higher, no BZ
SIM24 1 10−3 10−5 0.9375 2 Rg 4.0×10−7 2.0×10−8 as SIM21, β0 lower, stronger magn. field
SIM26 0.1 10−3 10−5 0.9375 2 Rg 2.0×10−7 1.0×10−8 as SIM24, β0 even lower, even stronger magn. field

Notes. Shown here: the simulation ID, the initial disk plasma beta, β0 (at the inner disk radius), the maximum floor density, ρflr, and internal energy, uflr, the Kerr parameter of the BH, a, the radius of the ISCO, Risco, and specific comments on the simulation runs, respectively. The Eddington ratios of these simulations for the defined HIGH-mass and LOW-mass system are obtained from the SED fits to the data for M87 as tabulated in Prieto et al. (2016) and for SgrA* in Narayan et al. (1998). The fits are obtained by fixing the values of Rlow = 1, Rhigh = 80 and an inclination angle of i = 17° when postprocessing the simulated data for each of the models.

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