Comparison of our best fit model, including Hills mechanism disruptions from both the NSC and CWD, with observations. Top: number of stars from our simulation compared to the observations for HVSs, evolved S-stars, and main-sequence S-stars. The error bars show the Poisson error on the predicted numbers from the model. Bottom left: cumulative distribution function of the visual Ks magnitude of S-stars for our simulations compared to the observations. Bottom right: cumulative distribution function of the semi-major axis of S-stars for our simulations compared to the observations.