Fig. 22.

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Cumulative distribution of the phase deviation rP, lit at the end of the observation obtained when adopting the literature period Plit instead of the Gaia period PGaia (see Eq. (6)). The sample of Gaia eclipsing-binary candidates that are also classified as eclipsing binaries in the literatures is shown by the filled grey histogram, and the sample which has literature cross-matches but with a classification other than eclipsing binary in the literature is shown by the red histogram.
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