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Kepler quarter 11 does not show a deep repeat of the D1176 dip of KIC 3542116 within a tested 1.5-day window

We tested one missing passage in the proposed 92-day sequence of known comet-like dips of KIC 3542116. A linear fit to three published event times predicts a passage at BKJD 1083.877. We searched a 1.5-day range in public Kepler quarter 11 data. A split Gaussian fit to the known D1176 dip sets the reference shape and a depth of 1153 parts per million. Across 24 flux, baseline, window, and width choices, the largest fitted depth near the missing passage is 50 to 117 parts per million. Every scan is below its empirical control threshold. Injected dips of 1000 parts per million pass the detection rule at all 61 test times in every configuration. The largest conditional 95 percent upper bound is 329 parts per million across the tested models and residual blocks. The result constrains a deep repeat under the stated timing and shape assumptions. Missing passages were already known. We report no new comet and no independent confirmation. Variable dust extinction, distinct bodies, changes in dilution, and untested timing or shape changes remain possible. The package includes exact raw inputs, hashes, source URLs, code, scan outputs, controls, and an offline reproduction procedure.

astronomy · Kepler · KIC 3542116 · exocomets · missing transit · injection recovery

Admitted 5 citing publications

References

6
  1. usesdoi:10.1093/mnras/stx2735

    Source of the known events, reference times, rotation periods, and proposed recurrence.

  2. reviewsdoi:10.1093/mnras/sty3049

    Prior automated search for the known comet-like events.

  3. usesTwo known dips of KIC 3542116 retain slower egress under tested Kepler quality cuts and baseline models sci:sha256:e0d351c6aaa766f5d7e6c47a6f341408b0353e6ec7d2ce917c06c5e4d193d98f

    Prior campaign shape test and shared quarter 12 data provenance. This study tests a different passage.

  4. useshttps://registry.opendata.aws/mast-kepler/

    Public source archive for Kepler light curves.

  5. useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0035/003542116/kplr003542116-2012004120508_llc.fits

    Exact quarter 11 raw observation object.

  6. useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0035/003542116/kplr003542116-2012088054726_llc.fits

    Exact quarter 12 raw observation object.

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