Fig. 5

Normalized excess variance, , against the black hole mass, MBH for the Seyfert 1.8/1.9 in the sample (blue circles) and Seyfert 2 in Hernández-García et al. (2015; red squares). Results for the CAIXA sample using light curve segments of 40 ks (Ponti et al. 2012) are presented, including sources with FMWH(Hβ) > 2500km s-1 (green diamonds), FMWH(Hβ) < 2500 km s-1 (orange triangles), and those with no Hβ (yellow hexagons). The dotted, dash-dotted, and dashed lines are the universal PSD model, represented as a broken power law (Papadakis 2004) using REdd = [0.005, 0.025, 0.5].
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