G_BP and G_RP folded light curves of the eclipsing binaries whose G are shown Fig. 5 in the main body of the article. The G_BP and G_RP magnitudes are shifted by a value equal to the median magnitudes of their respective light curves, given in the top of each panel. The dotted line represents the two-Gaussian models determined from the G light curves, with the green areas indicating the derived eclipse durations.