Fig. 6
Correlations between the absolute value of the [O III] wing component velocity, in abscissa, and other quantities. Top left: Eddington ratio; top right: logarithm of the bolometric luminosity (erg s-1); bottom left: logarithm of radio luminosity at 1.4 GHz (erg s-1); and bottom right: logarithm of the black hole mass (M⊙). RQNLS1s are indicated by red circles, RLNLS1s are indicated by blue squares. Black filled rectangles as in Fig. 5.
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