Fig. 3

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Folded eROSITA light curves of SXP 164 during ObsID 700 001 (top), 700003 (middle), and 710 000 (bottom), extracted in the 0.2–5.0 keV band. The best-fit sine function is overlaid. Phase 0 corresponds to the start of the first observation. The light curves from the first two observations are folded with the common period (163.89 s).

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