Notes. The parameters displayed here are the initial metallicity, Z, the mass of the stripped star, M_⋆, the mass of the helium core of the stripped star, M_Hecore, the luminosity, L, the stellar temperature, T_⋆ (at an optical depth τ = 100), the effective temperature, T_eff (at τ = 2/3), the effective surface gravity, log ₁₀g_eff, the stellar radius, R_⋆ (τ = 100), the effective radius, R_eff (τ = 2/3), the wind mass loss rate, Ṁ, the total hydrogen mass of the stripped star, M_tot,H, the total hydrogen mass at the end of the evolution of the stripped star, M_tot,H,f, the time during which the star is stripped, τ_stripped (the remaining life time after detachment from first Roche lobe overflow phase), the surface hydrogen mass fraction, X_H,s and the surface helium mass fraction, X_He,s. Unless stated otherwise we use the parameter values halfway through core helium burning which we define as X_He,c = 0.5. The helium core is defined as the most exterior mass coordinate where X_H < 0.01 and X_He > 0.1. We note that by construction T_⋆ ≈ T_eff,mesa, the surface temperature resulting from our MESA models. We use the values from our standard wind mass loss models and highlight our reference model in light gray.