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Can waveform residuals in gravitational-wave data distinguish the claimed effect from detector noise?

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Can waveform residuals in gravitational-wave data distinguish the claimed effect from detector noise?

This topic uses LIGO O3 Virgo 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.

Constraints from LIGO O3 data on gravitational-wave emission due to r-modes in the glitching pulsar PSR J0537-6910LIGO-Virgo-KAGRAGravitational wavescandidateRun : Define the concrete question
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Research questionCan waveform residuals in gravitational-wave data distinguish the claimed effect from detector noise?Source basisConstraints from LIGO O3 data on gravitational-wave emission due to r-modes in the glitching pulsar PSR J0537-6910Selected at—

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