The spatial distribution of match distances between extracted DR1 sources and the Pan-STARRS1 DR1 catalog, binned by the median match distance. We eliminate the “bullseye” pattern seen in Figure 6 of N. Aftab et al. (2024) and increase our astrometric accuracy, as illustrated by the smaller range of values in the colorbar (up to 2﹩\mathop{.}\limits^{\unicode{x02033}}﹩5 in DR0 versus 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩9 in DR1).