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Fig. 3.

image

Distribution of log(Lum[OIII]) for barred AGN galaxies (solid line), AGNs in pair systems (dashed line) and unbarred AGNs in the control sample (full surfaces). The D and p-values of the KS test between both samples (barred-agn, agn in pairs) and the CS is inset in the upper-left corner of the figure. The dotted vertical line represents the excess of Lum[OIII] for the barred-agn.

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