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Fig. 6.
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(a) SF-corrected radio luminosity. (b) Radio loudness. (c) Bolometric luminosity versus black-hole mass. (d) Radio luminosity as a function of bolometric luminosity. (e) Radio size (measured from FIRST) as a function of black-hole mass. All panels show radio Seyferts, OPARGs, and OPIRGs (sample sizes in legends).
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