Black Horizon LabScience AI
Do arrival-time residuals survive after detector-timing correction?

Selected topic

Do arrival-time residuals survive after detector-timing correction?

This topic uses KAGRA O3GK LIGO noise-subtraction work to test whether waveform residuals remain after detector noise is removed. The next pass should compare the residual claim against conservative data-quality limits.

Ultralight vector dark matter search using data from the KAGRA O3GK runLIGO-Virgo-KAGRAGravitational wavescandidateRun 1: Define the concrete question
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Research questionDo arrival-time residuals survive after detector-timing correction?Source basisUltralight vector dark matter search using data from the KAGRA O3GK runSelected at9 Aug 2026, 03:00

Run history

Runs for this topic

1 runs recorded
Run 1: Define the concrete questionALIVE

Do arrival-time residuals survive after detector-timing correction?

The source provides a relevant merger dataset, but it does not directly test delayed ringdown residuals.

Open report
Summary

The source provides a relevant merger dataset, but it does not directly test delayed ringdown residuals.

Hypothesis

Do arrival-time residuals survive after detector-timing correction?

Objection

The topic may still be broad enough that theory, template bias, and observation get conflated.

Next test

Which black-hole merger dataset gives the strongest baseline for delayed ringdown residuals?

Why it matters
  • It shows whether the topic can be tested with real observations instead of speculative language.
  • It keeps the analysis focused on ringdown data, residuals, and clean upper bounds.
  • It helps distinguish observational constraints from theoretical storytelling.
Evidence used
  • Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO The Astrophysical Journal Supplement Series

    It stays close to kagra and supports the concrete question pass.

  • An Interpretive Classification of Gravitational-Wave Ringdown Residuals -Residuals as Analytical Outcomes Rather Than Physical Signals Wiley

    It stays close to residuals and supports the concrete question pass.

  • Black Holes as Terminal Resonance Geometry in USP Field Theory Zenodo (CERN European Organization for Nuclear Research)

    It stays close to residuals and supports the concrete question pass.