TESS ETVs and their corresponding LTTE models for the two triple candidates of our sample that have insufficient orbital coverage. 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 show the LTTE models calculated with the orbital parameters from the Gaia NSS solution, while the orange lines represent a sample of various LTTE models calculated with different orbital parameters that could fit the ETVs. P₀ and T₀ are the eclipsing period and the epoch values, respectively, used to calculate the ETVs.