Same as Fig. A.3, but for three candidates in Sample 1GE of light curves modelled with one Gaussian and an ellipsoidal component. The top, middle, and bottom sets show cases with large (Gaia DR3 5310453356151345408), mild (Gaia DR3 4513043989925301760), and small (Gaia DR3 4052342222634008320) ellipsoidal component relative to the Gaussian depth. The secondary eclipse of the middle case may have gone undetected because of a lack of Gaia measurements at a phase of 0.5 apart from the primary eclipse.