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Fig. 3.

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Light curves of the J1544 counterpart candidate obtained with the OAN-SPM 2.1-m telescope and result of their modelling. Top: Light curves folded with a period of 2.724 h. The best-fitting model is shown with solid lines. Bottom: Fit residuals derived as the difference between the observed (O) and the calculated (C) magnitudes for each data point in terms of the magnitude error σ.

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