Same as in Fig. 4, but for NGC 4395. Open red squares in this case indicate the results of Vaughan et al. (2005). The solid lines indicate the best-fit log-linear model to the PSD_amp vs. E plot (left panel), the weighted mean α_high and ν_b (middle and right panels, respectively). The dashed line in the middle panel indicate the best-fit log-liner model with a slope equal to the slope of the bst-fit to the α_high − E data in NGC 4051.