Estimates of hydrogen- and fully helium-ionizing photon emission rates of individual stripped stars at Z = 0.002 from Götberg et al. (2018, Q₀ and Q₂, respectively). To estimate the ionizing emission from massive and hot stripped stars in a Z = 0.002 population, we fit a line to the stars with M_strip > 2 M_⊙. We then extrapolated this function up to stripped star masses of 17 M_⊙ to represent the emission from stripped stars that do not appear as WR type. For reference, we mark the Q₀ and Q₂ for an early O-type star and a hot WR star, respectively, according to models from Smith et al. (2002).