Sizes (r_bl), axial ratios ((b/a)_bl) and position angles (PA_bl) of barlenses obtained in this study are compared with those previosuly obtained by Herrera-Endoqui et al. (2015) or Laurikainen et al. (2011). Dotted lines indicate linear fits between the old and new measurements, whereas the dashed line stands for a unit slope. The labels indicate the slope and correlation coefficient of the linear fit. The galaxies that belong to the color subsample are indicated with an open symbol.