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 2: Extract the testable claim

Open dashboard Open source

Research questionDo arrival-time residuals survive after detector-timing correction?Source basisUltralight vector dark matter search using data from the KAGRA O3GK runSelected at13 Aug 2026, 03:00

Run history

Runs for this topic

2 runs recorded

Run 2: Extract the testable claimPROMISING

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.

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 hypothesis may still be too permissive unless the effect is separated from detector noise.

Next test

Which black-hole merger dataset provides the strongest constraints on 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

Gravitational-Wave Frequency-Comb Residuals: A Novel Probe of Quantum Structures Around Black Holes Zenodo (CERN European Organization for Nuclear Research)
It keeps waveform tied to one testable mechanism and a concrete observable.
An Interpretive Classification of Gravitational-Wave Ringdown Residuals -Residuals as Analytical Outcomes Rather Than Physical Signals Wiley
It keeps residuals tied to one testable mechanism and a concrete observable.
Ringdown tests of general relativity with spin-precession IOP Publishing
It keeps test tied to one testable mechanism and a concrete observable.

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.

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.