Galactocentric radial density profiles for the four quadrants of the Galactocentric projected sky. The crosses correspond to ten radial bins equally spaced in logarithm within 5 < r_q/kpc < 120. We also show the resulting fit for 100 samples drawn from the posterior distribution as the brown solid lines. The histogram corresponds to the posterior distribution of the break radius, r_br, and the dashed vertical lines are the corresponding 16th and 84th percentiles. The density profile of the full LSDR9 footprint, HAC-N, HAC-S, VOD, and Pisces are shown as the black, red, yellow, blue, and green lines, respectively.