Fig. 7.

Fraction of R > −0.6 as a function of stellar mass, (Mu − Mr) color, Dn(4000) parameter, or log(MBH) (a, b, c, and d, respectively), for barred AGN galaxies (solid lines), AGNs in pair systems (dashed lines), and unbarred AGNs in the control sample (dotted lines). Each bin for each sample contains a similar number of galaxies. The average number of galaxies in each bin is ≈93 for barred-agn, ≈270 for agn in pairs and ≈110 for CS.
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