Fig. C.1.
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Comparison of the Schwarzschild to the Kerr spacetime (left) and to the dilaton spacetime (right) in SANE, in thermal (left columns) and nonthermal emission (middle columns). The images are averages of 100 snapshots over 1 000 M simulation time (∼6 h for Sgr A*). A nonthermal electron distribution function has been applied in the jet sheath.
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