The redshift dependence of the SFR − δ_gal relation in the VUDS+ sample. The two panels are identical to the left panel of Fig. 5 except now the VUDS+ sample is broken up into two redshift bins with approximately equal numbers of galaxies. The meaning of the points and their associated uncertainties are identical to those in Fig. 5 as are the meanings of the vertical lines. As in Fig. 5, the SFR − δ_gal for all three VUDS+ fields are shown along with the combined sample. Left panel: SFR − δ_gal relation for the lower-redshift sample (2.0 ≤ z ≤ 2.7) and the right panel shows the relation for the higher-redshift sample (2.7 < z ≤ 5.0). The average stellar mass of each sample is given in the top-right portion of each panel and is effectively identical between the two samples. While a significant positive correlation between SFR − δ_gal exists in the lower-redshift sample, this correlation disappears when considering only galaxies in the Intermediate and Peak regions. In contrast, in the higher-redshift bin, the significant positive correlation is seen at all environments and increases in strength in the densest regions.