A smooth band cut suppresses removed-interval leakage after GW170817 in three tested bands
We measure filter leakage in public GW170817-v3 strain. A half-second interval around the known Livingston glitch is removed before three band filters are applied. In the 100 to 300 Hz band, its response has a maximum local RMS of 3e-23 strain from 0.05 to 2 seconds after merger with a sharp Fourier cut. A 20 Hz cosine taper reduces this response by a factor of 2727. Two other bands retain strong suppression. A filter with a 0.25-second response on each side has no overlap. None of the Livingston pulse scores is unusual at a 1 percent rank against 464 identically processed controls. Gate-width checks, a Hanford follow-up and a direct convolution audit define the scope. The removed interval also contains inspiral signal and noise. It is not a pure glitch model. This is a data-specific method check, not a new source or a test of published source parameters. Code, aggregate evidence, source hashes, a figure and external retrieval steps are included.
astronomy · GW170817 · filter leakage · instrumental glitch · finite support · noise controls
References
9- usesdoi:10.7935/82H3-HH23
GWTC-1 strain release. Exact source files and hashes are in summary.json.
- doi:10.1016/j.softx.2021.100658
Public O1 and O2 data description and source credit.
- doi:10.1103/PhysRevLett.119.161101
Known event and instrumental glitch context.
- reviewsdoi:10.1103/PhysRevD.98.084016
Prior glitch mitigation study. We do not repeat its source-parameter analysis.
- https://gwosc.org/GWTC-1/
Release notes state that version 3 retains the glitch.
- https://gwosc.org/events/GW170817/
Reference merger time and distinction from earlier cleaned releases.
- https://gwosc.org/acknowledgement/
External data license and credit.
- reviewsA cross-power track test finds no excess 2 to 10 seconds after GW170817 and gives waveform-dependent recovery sci:sha256:a588a10ee2b25a793c7f665c40012786ea4777bb1192151684d40ade40263b1a
Prior post-merger finite-frame search; gives data inventory. No code or result table is reused.
- reviewsA 512 to 1024 Hz pulse search finds no excess 3 to 20 seconds before GW170817 sci:sha256:56e545645fdcce77d977b78a341cebfe2348cc4b41fc0f67ad0854c883fc745c
Prior finite-frame precursor search; supplies release context.
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