Sixteen barlens galaxies common with Méndez-Abreu et al. (2018) and this work are shown in the V/σ−ϵ plane. The parameters refer to values measured within one R_e of the bulge (see Table 2 in Méndez-Abreu et al. 2018). They are corrected for pixelation and resolution effect (as explained in the original paper). The solid line shows the expected relation for rotationally flattened oblate spheroids seen edge-on, following the approximation given in Kormendy (1982). The dashed line () shows the region in which the slowly rotating bright ellipticals fall in the study by Emsellem et al. (2011; see their Fig. 6a). Also indicated in the figure are the Milky Way (MW) bulge (red cross) and NGC 4565 (star) using the values from Rich et al. (2008).