Explain the detector-specific discrepancy in spin orientation inference for GW231123
Identify and account for the cause of the discrepancy between LIGO Hanford-only and LIGO Livingston-only analyses in the inferred spin orientations for GW231123, determining whether it arises from data characteristics, instrumental effects, or waveform-model limitations by reproducing or eliminating the effect with controlled injections and diagnostics.
References
The differences between the results in the two detectors could potentially be explained by lower signal power in LIGO Hanford (such that precession is not measurable), but we have not been able to reproduce this discrepancy between detectors with injections in zero-noise, for example, of the NRSur waveform at its maximum-likelihood parameters.
— GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$
(2507.08219 - Collaboration et al., 10 Jul 2025) in Appendix B, Source properties