Phase-folded light curves (in green) from each instrument (or sector in the case of TESS) with the best-fit transit model for TOI-375 b derived using juliet. Also shown is the potential single transit event (in blue) of one of the outer planets on TESS sector 2. Data points are shown in their original time sampling (small green or blue points) and binned in phase with 6 minute intervals (white markers). The solid black line represents the best-fit transit model. We do not include the transit of TOI-375 c in the final model as there is not enough evidence to support that it has a true planetary origin.