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Fig. A.1.

Fig. A.1. Refer to the following caption and surrounding text.

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Observed multi-band and multi-period photometry for the star Gaia DR3 2935152926080940544 with the best-fit light curve models. The points represent the observed magnitudes, and the curves represent the best-fit light curve for each photometry band. The horizontal dashed lines are the mean magnitudes for each best-fit model of each band. To create the multi-band light curve model for this star, we used OGLE bands I (purple) and V (yellow), and Gaia bands G (green), BP (blue), and RP (red).

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