Fig. 15
RBLR versus L, from Bentz et al. (2009). Shown is a zoomed portion containing the two sources PG0003+199 and Ark120. For PG0003+199 we used RHβ = RHα/1.37 (Sect. 3.1.2). The new measurements shift both objects clearly outside the range of the previous errors bars and about a factor 2 closer to the dashed line that is the fit with a slope α = 0.519 obtained by Bentz et al. (2009).
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