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Fig. 3

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TESS ETVs and their corresponding LTTE models for two of our validated triple candidates. Delay times calculated from primary and secondary eclipses are indicated with red and blue points, respectively, while their averaged values for the same orbital cycles are shown with black points. The green dashed lines denote the LTTE models calculated with the orbital parameters from the Gaia NSS solution, while the blue lines represent our LTTE models after modifications in the orbital parameters. P0 and T0 are the eclipsing period and the epoch values, respectively, used to calculate the ETVs.

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