Fig. 4
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Orbital periods of double eclipsing binaries of the three largest samples: the sample from OGLE (Zasche et al. 2019), the sample from TESS by Kostov et al. (2022) and Zasche et al. (2022b), and the ZTF sample from this work. Here Pshort is defined as the shortest period of A and B, and Plong as the longest period of A and B.
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