Finite post-peak detector-frame windows for GW250114 yield a stable common-remnant Kerr interpretation after calibration on synthetic waveforms and robustness checks.
For each fixedWandA, define the total detector-frame remnant radii R tot,A,W M (q;α) = R 0,A,W M + R stat,A,W M (q;α),(J.13) R tot,A,W χ (q;α) = R 0,A,W χ + R stat,A,W χ (q;α)
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Deterministic Trust Regions for Finite-Window Black-Hole Spectroscopy in GW250114
Finite post-peak detector-frame windows for GW250114 yield a stable common-remnant Kerr interpretation after calibration on synthetic waveforms and robustness checks.