Specific star formation rate as a function of v/σ for all subhalos in five EAGLE simulations. Vertical lines show the selection boundary between pressure-dominated and rotation-dominated galaxies (i.e., v/σ = 0.5). Horizontal lines show another boundary that separates quiescent and star-forming galaxies (i.e., sSFR = 2 × 10⁻¹¹ yr⁻¹). The numbers indicate the fraction of galaxies in each area among the entire sample with log(M_*/M_⊙) > 9. White circles show the median sSFR at each v/σ bin. The error bar indicates the 1σ standard deviation of the galaxies in each v/σ bin.