Non-host-subtracted g-band light curves of five TDE candidates showing significant optical flares. The x-axis shows time after eROSITA peak in days, so x = 0 corresponds to the peak eROSITA detection for each source. The summary of observational information is provided in Table C.1. The individual-host-subtracted light curves are showin in Fig. C.3. The optical flare of J0744 is too faint to be distinguished in a non-host-subtracted light curve and is only shown in the host-subtracted plot.