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Fig. 2


Maximum phase gap versus period for all OGLE-III LMC eclipsing binaries. Folded light curves with a clumped distribution of their phases (clumpiness above 0.75 on a scale between 0.5 for a uniform-like distribution to 1 for a highly clumped distribution) are shown as black crosses, while the other folded light curves (clumsiness below 0.75) are shown as gray filled circles.

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