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Fig. 12.
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Period-morphology distribution of the OGLE EBs, the foreground (red) and the background (blue) EBs. The foreground binaries mimic the distribution of OGLE binaries surprisingly well, and the distribution of the found background systems shows a stronger peak in a well-defined phase range (0.6 < C < 0.9 and 0.2 < P < 0.5).
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