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Fig. A.3

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Relative peak height and S/N of all objects including double eclipsing binary candidates and test objects. Left: Relative peak heights A and B for all objects. Middle: S/N A and S/N B results for all objects. Right: S/N B and relative peak height B of all objects. We see that quadruples can have a wide range of RPH and S/N values. However, this also means that more can be found at values of RPH < 10 & S/N <10.

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