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The 2025 Kepler-451 TESS table has two used rows for 888 eclipse events

We checked the public machine-readable Table 1 of Er et al. (2025). Its 2,382 TESS timing rows describe 1,489 primary eclipse events. Of 2,376 rows marked for use, 888 events have two times and 600 have one. Three published linear clocks and a test based only on time gaps give the same event groups. The five published TESS means agree with averages over all retained rows to within 0.001 s. Giving each event equal weight changes a mean by at most 0.216 s. Selecting the smaller or larger stated error in each event changes a mean by at most 0.551 s. Exact bounds over every choice of one recorded time per event have a maximum width of 8.147 s. The published errors are 21.74 to 24.79 s. The stated error rule does not reproduce these errors from the retained rows. A rule that uses the scatter of individual residuals gives values within 0.009 s. The table has no cadence labels, so it cannot identify which row the authors intended to retain. This audit supplies an event record, source data, code, figures, and independent checks. It does not establish or reject a planet. The method wording was checked in the June 2026 author version.

Kepler-451 · TESS · eclipse timing · data audit · circumbinary planets · reproducible research

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References

7
  1. challengesdoi:10.3847/1538-4357/ae1029

    We audit its public Table 1. It retains two rows for 888 used TESS eclipse events. This differs from the one-measurement rule described in the June 2026 author version. We reproduce the five published centers and bound changes in their weights. We do not test or reject its companion models.

  2. usesdoi:10.48550/arXiv.2606.26817

    We checked the method description and printed linear clocks in version 1, posted on 25 June 2026. The source table is the journal revision1 file.

  3. usesdoi:10.1093/mnras/stac357

    Prior Kepler-451 planet timing study. Its printed linear clock supplies an independent check of the event groups.

  4. usesdoi:10.1117/1.JATIS.1.1.014003

    TESS mission description. One public SPOC light curve shows the repeated event directly.

  5. usesdoi:10.1038/s41586-020-2649-2

    NumPy supports the independent calculation and summary statistics.

  6. usesdoi:10.1109/MCSE.2007.55

    Matplotlib makes the figures.

  7. usesdoi:10.3847/1538-4357/ac7c74

    Astropy reads the original TESS FITS data for the example figure.

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