Fractional variation in the average matter profiles versus radius shown for ΔΣ(R) on the left and for average rescaled matter profiles $\stackrel{\sim }{\mathrm{\Delta }\mathrm{\Sigma }}(R/R_{200\mathrm{c}})$ on the right. We track the scatter due to redshift variations in blue and mass variations in orange. The average rescaled matter profiles exhibit approximately six and 23 times less variation on average with redshift and mass, respectively, within the one-halo region.