G^{SB − rP20S} vs. M20 measured in the rest-frame optical (left panels) and Lyα (right panel) of the original LARS galaxies (squares). LARS-LAEs are indicated with open circles. In each raw the colour scale corresponds to an integrated physical property derived in Paper II (vertical colour bar). From the top raw the integrated physical properties are stellar mass, Lyα escape fraction, dust-corrected specific star formation rate, nebular reddening, and age. The dashed lines indicate the regions of separation between merging system, normal galaxies, and bulge-dominated systems as presented in Figs. 13 and 14.