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Table 2.

Isolated galaxy simulations suite.

fEdd(t) Mα(t)
qcrE Variable Variable
qcrC 1 4.975 ⋅ 105 M

Angular pattern

qcrf f(a(t);θ)
qcra0 f(a = 0.01; θ)
qcriso 1

Notes. Main features of the isolated galaxy simulations. (left) The dimensionless accretion rate and subgrid disk mass for the qcrE and qcrC simulation sets. We note that while subgrid disk quantities are evolved only in qcrE simulations, the MBH mass and spin evolve according to the prescriptions detailed in Appendix A in both simulation sets. (right) The AGN radiation angular patterns used in each simulation set.

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