Visualization of the properties of the gold sample of 30 BL Her models that match the best with BL Her stars in the LMC. Top panels: Histograms of the distribution of the BL Her models as a function of stellar mass (M/M_⊙), stellar luminosity (L/L_⊙), metallicity ([Fe/H]), effective temperature (T_eff), and the convection parameter sets, respectively. The location of the subset of BL Her models is also depicted on the Hertzsprung-Russell diagram; the red and blue edges of the instability strip are estimated from the linear stability analysis from Paper I. Bottom panel: PW and PR relations of the 30 BL Her models, respectively.