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Fig. 5.
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Comparison of mm-wave and X-ray luminosities for RXJ1131 (blue) and local AGNs (Behar et al. 2018; Ricci et al. 2023). The mm-wave/X-ray luminosity ratio in RXJ1131 is consistent with predictions for coronal emission (L100 GHz/L2 − 10 keV = 10−4.5, orange line; Guedel & Benz 1993; Krucker & Benz 2000).
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