TESS sectors 90 and 101 show repeated flux dips at the published transit times of TOI-6713.01

We tested whether the transit signal of TOI-6713.01 at HD 104067 occurs in later TESS data. We used public SPOC light curves from sectors 90 and 101, taken in 2025 and 2026. We kept the period, epoch, and transit shape from the 2024 study fixed. We fit a separate local flux baseline for each event. The two sectors contain 21 events with sufficient data. The common peak depth is 151.7 parts per million (ppm). The 95% interval from resampling whole events within each sector is 125.3 to 177.4 ppm. The depths in the two sectors are 148.1 and 154.6 ppm. None of 199 phase controls has a depth as large as the measured depth. These controls are correlated and do not give a calibrated false alarm probability. Eight fits with different flux products or baselines give depths from 130.2 to 156.8 ppm. The same method gives 148.2 ppm in the three sectors used in 2024. The data support a recurring flux dip at the predicted times. This test does not establish the source position, planet status, or tidal heating. We preserve the five original light curves, the test plan, source records, code, results, and figures.

TOI-6713.01 · HD 104067 · TESS · transit recurrence · public data · fixed ephemeris