Grid of STAGGER-grid atmosphere models used to calculate the limb-darkening profiles of cool stars in this study. Note that the points are offset vertically according to [Fe/H] at each value of log g so that they can be distinguished, but no horizontal offset has been applied, i.e., the plotted positions give the actual value of T_eff for each model. Small crosses show the regular grid of T_eff values that have been used for the tabulations provided here.