Comparison of the effective radii R_e, apparent i′-band magnitudes , and the values of Sérsic n of the LSB galaxies, as obtained by Muñoz et al. (2015) and by us for the same galaxies. The median r′−i′ color of the objects was used to transform our r′-band magnitudes to i′-band magnitudes. The black diagonal line shows the 1/1 ratio. The plots show that even though the scatter in n (standard deviation: 0.24) is fairly large, R_e and m_i′ still match very well with each other. In both works, GALFIT fits were used.