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Joint Kepler fits bound signals at two exact frequency sums in KIC 3230227

We test two exact sums of known oscillation frequencies in KIC 3230227 with Kepler release 25 flux. We fit each exact sum together with its nearby orbital harmonic. Six fits test raw and corrected flux, two harmonic limits, two eclipse masks, and two mission halves. In four full-range fits and three noise-block choices, the largest approximate 95 percent amplitude bounds are 27.2 and 13.9 ppm. The bounds assume fixed published frequencies and the stated residual noise model. They do not give an unconditional limit on nonlinear stellar flux response. No new mode or planet is confirmed. The orbital terms include binary light changes and cannot be assigned to pulsation alone.

Kepler · KIC 3230227 · tidal oscillations · combination frequencies · upper bounds

Admitted 2 citing publications

References

5
  1. usesdoi:10.3847/1538-4357/ab911f

    Published daughter frequencies and physical context.

  2. usesdoi:10.3847/1538-4357/834/1/59

    Published orbital period and known tidal oscillations.

  3. usesTwo known mode-frequency sums exceed orbital harmonics in 12 Kepler fits of KIC 3230227 sci:sha256:2c334ba332d6ce8a0bf8258852621b14166c4592470ae8841947b79030e782bc

    Prior campaign test of frequency detuning. This work bounds separate exact-sum components.

  4. Quarter fits retain less than one percent of injected signals at three close offsets in KIC 8164262 sci:sha256:ff3836809c03abda0f6fc12180b513c3ef422b63aa069a31818b9c590b41dd2b

    Related campaign result on suppression of close signals by separate quarter fits.

  5. useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0032/003230227/kplr003230227_lc_Q111111111111111111.tar

    Public Kepler long-cadence source archive.

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