Panel H: LARS sSFR(Hα) and burst fraction , color-coded by EW(Hβ). Panel I: comparison between LARS and BCG burst fractions, cutoff radii [kpc] and B-band cutoff surface brightness. Panel J: LARS clumpiness S vs. median M/L_B ratio, color-coded by . Panel K: M20 vs. Gini coefficients, color-coded by . The Lotz et al. (2004) sample contains E/S0-Sd (gray open circles) from Frei et al. (1996), SDSS u-band selected galaxies (gray filled circles) and dIrr (open black circles) from van Zee (2001). Panel L: as in panel K but for clumpiness S vs. asymmetry A. Panel M: asymmetry A as a function of B-band isophotal surface brightness μ_B. The average from all galaxies is indicated with a dashed black line. Panel N: central surface brightness μ₀ and scale length [kpc] from the 1D fit (Sect. 3.6). Panel O: absolute B-band magnitude and 1D fit scale length. All panels: shaded area is the confidence interval of the linear regression (blue solid line). BCG photometry has been converted from Vega mag to AB mag. Galactic extinction and surface brightness dimming has been applied. Numbers inside markers indicate the LARS number.