Same as Fig. A.3, but for three candidates in Sample 0GE (light curves modelled with only a cosine). The first two examples show the most common cases of faint candidates, with (top case, Gaia DR3 5923298253884922624)and without (middle case, Gaia DR3 4037337565429141376) clear confirmation of the variability in the G_BP and G_RP light curves. The bottom example shows a relatively rare case (in this sample) of a bright candidate (Gaia DR3 5236421790821776256).