Plots of the azimuthally averaged, stellar surface number densities as a function of projected distance from Sgr A* for all stars in our sample (black), red giants (red), and early-type star candidates (green), with 9.75 <  [2.25]  < 12.25. The densities were determined in annuli of variable width, chosen such that each one contained a fixed number of stars (5 stars for the early-type star candidates, and 15 stars for the entire sample and the red giants). Data points at 10″ ≤ R_SgrA∗ ≤ 60″ were used for power-law fits of the radial profiles for our entire sample (black line), red giants (red line), and early-type star candidates (green line). The green dashed line represents a power-law fit to the densities of the early type candidates, including those at R_SgrA∗ ≤ 10″.