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Fig. 3

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Sparse photometry from surveys. The left panels show the comparison between the light curve predicted by the convex shape model (red points) and observed photometric data (blue points) from ATLAS in c and o filters and Gaia. The brightness in relative flux units is plotted against the solar phase angle to see the phase curve. The three panels on the right show the difference between observed and modeled brightness and the values of root mean square residuals.

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