Coalescing Compact Binary Parameter Estimation with Gravitational Waves in the Presence of non-Gaussian Transient Noise
This study quantifies how non-Gaussian transient noise glitches in LIGO detectors bias the parameter estimation of compact binary coalescence signals, revealing significant distortions in mass, spin, and sky position—particularly when glitches occur shortly before the merger—and establishing time-separation thresholds to identify when glitch subtraction is necessary for unbiased results.