The 95.4% (magenta in the online version) and 99.7% (lighter regions, cyan) confidence areas in the log r₀ − log ρ₀ plane and in the log r₀ − log M_∗ plane relative to the rotation curve fit using a core model and the BVI mass map. In the top panel, the dash-dot line indicates the most likely stellar mass according the synthesis models, which rely on the BVI colors. There are no core models in the 68.3% confidence area for the BVI mass map and no acceptable core models for the BVIgi mass map down to the 99.7% level. The solid line in the bottom panel indicates the inverse log ρ₀ − log r₀ correlation found by Donato et al. (2009).