Fig. 12
RBLR versus L, using data from Bentz et al. (2009), Denney et al. (2010), Doroshenko et al. (2012) and Grier et al. (2012). As a red dot we included our results for ESO 399-IG20. Shown is a zoomed portion containing ESO 399-IG20. The solid dotted line show a fitted slope α = 0.519. ESO 399-IG20 lies close to the expected slope.
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