Fig. 12
Comparison between periods measured in the present work and in Henderson et al. (2011). Gray circles show the periodic stars in common between the two works. Stars with the same period measured in both works fall over the red dashed line. Red circles show the eclipsing binaries candidates from Henderson et al. (2011). Continuous black lines show 1 day aliasing paths and dashed black lines show the path for harmonics.
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