v/σ_m, corr versus galaxy mass (top left) and effective radius (R_e, top right), specific star formation rate (sSFR, bottom left) and the surface density of star formation rate (Σ_SFR, bottom right). Both the sSFR and Σ_SFR are corrected for extinction. The colours and symbol signs are the same as in Fig. 12. Two galaxies, J1140 and J1340 are missing in the top- and bottom-left plots, as no masses are derived in the SDSS database. The vertical dotted lines in the bottom right panel are those galaxies where the Paα or Brγ emission does not cover the entire galaxy, therefore potentially resulting in underestimating v_rot. The location of the triangle shows the position of the galaxies with 2 times higher v_rot (Sect. 6.1). The horizontal dotted line shows the deviation between dispersion and rotationally dominated galaxies (, Schreiber & Wuyts 2020). Over-plotted are sample from the literature, with symbols identical to Fig. 2.