Same as Fig. A.3, but for three candidates in Sample 1G of light curves modelled with only one Gaussian. The top set (Gaia DR3 5524068296237910272) shows a case where the period is probably a factor of two too small, the second set (Gaia DR3 3033226683222463872) shows a case where observation may be missing at the phase window of the second eclipse, and the third case (Gaia DR3 5541461814286341632) illustrates a case where the lack of sufficient phase coverage within an eclipse leads to an overestimation of the eclipse depth.