Example G light curves (top panels in each set) and G_BP and G_RP light curves (bottom panels in each set) of sources in Sample 2G-A modelled with only two Gaussians. The G_BP and G_RP magnitudes are shifted by a value equal to their median magnitudes, the values of which are given in the panel. The two-Gaussian model obtained from the G light curve is superposed as a dotted line in both panels of each set. The green areas indicate the derived eclipse durations. The top set is for the circular candidate Gaia DR3 5632871775033302656 and the bottom set is for the eccentric candidate Gaia DR3 2059784985669541760.