Comparison of ~18,000 stellar mass estimates from our VAC and GSWLC 2 catalogs (top panel) and difference in stellar mass estimates (bottom panel). The 1:1 and 0.2 dex lines are marked with black solid and dashed lines, respectively. The linear fit (red line) and the Pearson correlation coefficient are reported in the legend. The bottom panel shows the dependence of the stellar mass residuals on the availability of WISE photometry expressed by FLAGINFRARED: the scatter increases when WISE photometry is readily available.