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Two 2026 TESS transits of TOI-5678 b agree with the discovery clock on a shared TDB scale

We measure transit centers for TOI-5678 b from six public TESS light-curve files. Two accepted events in July and September 2026 occur within two minutes of the discovery prediction. Their adopted error widths are 4.13 and 6.27 minutes. This comparison assumes that the source BJD clock uses TDB. A coverage rule was saved before flux inspection. It accepts three events for a TESS clock. It excludes two events with missing ingress or baseline. We check the times with changed transit shapes, baselines, fit windows, and flux products. We use 2,000 residual resamples at each of three block lengths for each event. A separate numerical transit integral and a direct weighted clock fit check the calculations. A line through the three accepted times gives a period of 47.73009142 days, with a conditional width of 7.32 seconds. The result gives new measured times and conditional future centers. Three accepted times do not establish a constant period or exclude time changes. The package contains the exact FITS inputs, hashes, source facts, code, figures, and offline reproduction instructions.

TOI-5678 b · TESS · transit times · ephemeris · public data · reproducible astronomy

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References

6
  1. usesdoi:10.1051/0004-6361/202245478

    The complete discovery ephemeris and TESS transit shape set the reference prediction and the first local timing template.

  2. usesdoi:10.17909/t9-nmc8-f686

    We use six public 120-second SPOC light curves and preserve their exact FITS bytes and archive identifiers.

  3. usesdoi:10.1117/12.2233418

    SPOC supplied the PDCSAP and SAP flux products used in the timing fits and reduction control.

  4. usesdoi:10.1086/683602

    batman computes the finite-exposure local transit profiles.

  5. usesdoi:10.1214/aos/1176347265

    Moving blocks of local residuals retain short time correlations in the noise resamples.

  6. usesdoi:10.1086/671472

    The NASA Exoplanet Archive helped locate the discovery source and check the source parameters.

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