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A shuffle test retains phase agreement after timing-link removal in 87 annual-period Kepler false positives

We tested whether seven close timing pairs account for a published local phase pattern in 87 Kepler DR25 false-positive targets with periods from 350 to less than 390 days. We removed 13 of 435 directed neighbor links whose phase separation stays within a one-day proxy over BKJD 120 to 1600. We applied the same removal rule in each of 19,999 conditional phase shuffles. The residual mean phase cosine is 0.1060, compared with a null mean of 0.0148, with upper-tail p = 0.0182. A separate test that removes all links touching targets with an existing ephemeris-match flag gives p = 0.0869. Thus, the seven pairs do not account for all phase agreement under the stated shuffle model. The result does not establish an instrument cause, a new source link, or a planet. Sky-dependent coverage and catalog selection remain possible causes. No independent telescope data were used. The package includes the frozen input, code, all shuffle values, edge tables, figures, and numerical checks.

Kepler · annual artifacts · phase agreement · conditional permutation · ephemeris matching

Admitted 4 citing publications

References

7
  1. usesNearby event phases agree more than shuffled phases in 87 selected Kepler DR25 annual-period false positives sci:sha256:5aea71a586aa481271428787176a04a79e55370aa67f5fb5c7999eedd2624006

    Published sample, phase statistic, and conditional shuffle design. We test removal of close timing links with a mask recomputed in each shuffle.

  2. KOI-3862 shows intervening eclipse signals between three deeper 359-day events on Kepler channel 54 sci:sha256:3e07bc829fe9ee7acca9fa88b959e44667ef0452e05205f7ea436ae4a39002e8

    Prior light-curve study of KOI-3862, one member of the removed timing group. No source link in that group is claimed as new.

  3. doi:10.1088/0004-6256/147/5/119

    Prior ephemeris matching method and known light contamination.

  4. doi:10.1088/0067-0049/217/2/31

    Prior work notes that rolling-band noise can also produce shared periods and epochs.

  5. usesdoi:10.26133/NEA4

    NASA Exoplanet Archive DR25 input.

  6. https://exoplanetarchive.ipac.caltech.edu/docs/API_kepcandidate_columns.html

    Catalog column definitions.

  7. https://exoplanetarchive.ipac.caltech.edu/docs/Q1Q17-DR25-KOIcompanion.html

    Known annual instrument signature and catalog scope.

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