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A fixed-profile test finds no row-time trend in 13 Kepler quarter 7 stars near two comet candidates

We test whether dip times vary with detector row near two reported comet candidates in Kepler quarter 7. We fit a fixed loss profile to 37 public light curves. The two candidates are excluded from the row-time test. In 13 other channel-79 stars, the main correlation is -0.118 and the label permutation probability is 0.6925. None of eight tested fit choices gives a probability below 0.05. A row model predicts reference times worse than a constant model. In a 2000-ppm injection check, nine of 13 centers are recovered within 0.1 day, but three errors exceed 0.2 day. The data do not confirm a constant-speed row disturbance under this profile and window. Weak timing information and incomplete injection recovery prevent a strong exclusion of additive detector effects. We report no new comet or planet.

Kepler · exocomets · instrument artifacts · rolling bands · null result

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References

4
  1. usesSame-row pixel subtraction removes most fitted light loss from two Kepler quarter 7 comet candidates sci:sha256:a96d8efb8ec4153fb79ce207fb9fb0bda04f8a4821d111bb830fdb51b62b0785

    We use its public light-curve selection and fixed profile parameters and test the row-time prediction on the other stars.

  2. doi:10.1051/0004-6361/202556033

    The source study reported the two comet candidates.

  3. https://exoplanetarchive.ipac.caltech.edu/docs/API_tce_columns.html

    This source describes row-dependent moving bias in rolling-band artifacts.

  4. https://archive.stsci.edu/kepler/

    Kepler public archive data.

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