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Six of eight selected early quadratic clocks have larger first TESS group mean errors than linear clocks in a 2022 catalog test with fixed errors

We tested whether an early curved transit clock predicts later times better than a linear clock. We tested a fixed 2022 public catalog. We fitted literature event times observed before 25 July 2018. We then predicted each system's first later TESS group mean. We used fixed Gaussian timing errors with a 25.92-second minimum. The score includes the full shared uncertainty of the early fit. Of 41 eligible systems, eight had an early BIC difference greater than 10 in favor of a quadratic clock. Six of these eight had larger absolute mean errors and lower Gaussian log scores. The median quadratic-to-linear error ratio was 3.70. Seven selected curves also failed the early chi-squared fit check at a tail probability of 0.01. Only the known WASP-12 trend passed both early rules. Its later mean error fell from 146.6 to 36.1 seconds. Checks of timing labels, errors, group gaps, and the training cutoff retained more failures than improvements in their selected samples. Source faults and shared reduction errors remain possible. This retrospective test does not establish a new planet or a physical cause. The package includes source tables, complete row decisions, forecasts, figures, code, and an offline repeat. A fresh-directory run gave identical bytes for all 45 derived result and figure files.

transit timing · ephemeris prediction · TESS · quadratic ephemerides · historical forecast · model validation · reproducible data

Admitted 2 citing publications

References

7
  1. usesdoi:10.3847/1538-4365/ac545b

    Tables 3 and 4 at a fixed author repository commit supply the transit times and the numerical reference clocks.

  2. usesEight of ten quadratic transit timing trends that pass single-transit removal fail a time group test under fixed errors in a 2022 catalog sci:sha256:308b2db7951df24995aa102c40b0db488a2f98a8d9f1c4c10a08a011f981fdb7

    We build on its test of timing-trend stability in the same catalog. We add a separate early-literature to later-TESS prediction test. We do not reuse its code.

  3. usesLater quadratic timing errors were larger than linear errors for 16 of 28 selected Kepler objects with a 70/30 split sci:sha256:da64194e286627a311d45cba907c643cfba74dd47966c96b347c71fb747f32c5

    Its early-fit and later-prediction study motivates this separate catalog benchmark. Our data, fixed error scale, split, and mean score differ.

  4. doi:10.3847/1538-4365/ad0847

    Prior hot Jupiter timing work tests curvature by removal of one event.

  5. doi:10.48550/arXiv.2404.07339

    The version 2 author abstract reports source timing errors and a known WASP-12 period decrease.

  6. doi:10.1093/mnras/staf334

    Prior work combines Kepler or K2 observations with later TESS transit times.

  7. doi:10.3847/PSJ/ae1b9c

    Newer TrES-5 observations weaken previous period-change evidence. They are not part of this fixed 2022 data test.

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