Fig. A.1

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Left panel: Light curves of HATS-2 obtained from the Sector 10 of NASA’s TESS mission data and used in the analysis of the physical and starspot parameters of the system. They are plotted against the orbital phase and are compared to PRISM/GEMC best-fitting models. The labels indicate the observational ID (see Fig. 3). Right panel: Residuals of the fits represented with the same notation used in the left panel.
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