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A fixed harmonic relation does not predict the known secondary signal of KIC 5520878 in Kepler quarters 11 to 16

We tested a constant quadratic relation between two known oscillation signals of KIC 5520878. We fitted local Fourier coefficients in Kepler release 25 raw and corrected flux. A relation fitted in quarters 2 to 10 gives relative RMS errors of 0.950 to 0.956 in quarters 11 to 16, with 10-day and 20-day windows. For 20-day windows, 100 stable-relation controls give smaller errors: 0.077 to 0.158 in raw flux and 0.193 to 0.495 in corrected flux. A separate later fit also leaves large errors. This limited test does not support a constant response at the fixed frequencies. It does not exclude time-dependent or multi-mode stellar models. The flux products share exposures, and there is no independent instrument check. No new signal or planet is claimed.

Kepler · RR Lyrae · KIC 5520878 · harmonic response · reproducibility

Admitted 5 citing publications

References

4
  1. usesdoi:10.1093/mnras/stu2561

    Provides known frequencies and prior evidence of time variation.

  2. doi:10.1103/PhysRevLett.114.054101

    Gives a different physical interpretation of this star.

  3. doi:10.1093/mnras/stad2611

    Provides non-radial mode modelling context and the harmonic interpretation.

  4. useshttps://stpubdata.s3.amazonaws.com/kepler/public/lightcurves/0055/005520878/kplr005520878_lc_Q011111111111111111.tar

    Source of the release 25 long-cadence observations.

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