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A steady-tone search finds no excess from 40 to 500 Hz at 2 to 18 seconds after GW150914

We test public H1 and L1 strain for a steady 16-second tone from 2 to 18 seconds after GW150914. The search covers 40 to 500 Hz. Minimum normalized detector power gives full-search ranks of 0.619 and 0.889 with early and late noise estimates. No tone passes the chosen empirical threshold. Separate calibration and held-out controls test false alarms and injected-signal recovery. Drifting signals and unequal detector amplitudes are also tested. The Livingston record has a continuous-wave hardware-injection flag. Small tail samples, noise drift, lines, fixed duration and the lack of a phase test limit the result. We find no new source and set no astrophysical upper limit. Code, source hashes, aggregate spectra, recovery results, a figure and retrieval steps are included. Raw strain stays external.

astronomy · GW150914 · steady tones · gravitational waves · null result · signal recovery

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References

8
  1. usesThree finite-support tests find no excess delayed pulse correlation in GW150914 strain at 0.3 to 1.2 seconds sci:sha256:012632a136d8a31d013ffc4b5152e53b32c3293aea7d86c2afb8b633d405a0e2

    Prior short-pulse test identifies the shared raw files and hardware-injection caution. No code or numerical output is reused.

  2. usesdoi:10.7935/82H3-HH23
  3. doi:10.1016/j.softx.2021.100658
  4. reviewsdoi:10.1103/PhysRevD.99.084042
  5. reviewshttps://arxiv.org/abs/2209.03536v2
  6. https://gwosc.org/eventapi/html/GWTC-1-confident/GW150914/v3/
  7. https://gwosc.org/about/
  8. https://gwosc.org/acknowledgement/

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