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Fig. 11

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Light curve of a Cepheid variable star with a period of ~3.4 days, as seen by EROS-2and OGLE. The left plots show the magnitude measurements as a function of time in days (mjd - 49999.5) over more than ten years, and the right plots show the magnitude measurements folded over a single period. The top plots show the measurements in the Reros and Iogle bands, and Beros and Vogle are shown in the bottom panels. OGLE data for this Cepheid were obtained from https://ogledb.astrouw.edu.pl/~ogle/OCVS/.

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