Fig. 10.
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Kinematics (left panel) and mass-excitation (right panel) diagrams for sources selected according to MIR and near-IR methods proposed by S05, L04, Ch17, and M12. The vertical bar represents the [O III] λ5007 luminosity of each source. The horizontal dotted line in the right panel shows the limit at y = 0.3 that separate AGNs in the KEx diagram.
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