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Fig. C.1.
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LCs of the O’Connell EB candidate ZTF17aaadztm in the four filters used in this study: ZTF r, ZTF g, ATLAS c, and ATLAS o. The gray line corresponds to the best fit using our model (Eq. 5). The period of the star is also shown at the top of the figure, along with its ZTF ID.
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