A semicoherent glitch-robust continuous gravitational wave search
arXiv:1805.03314 · doi:10.1103/PhysRevD.98.063011
Abstract
Continuous gravitational-wave signals from isolated non-axisymmetric rotating neutron stars may undergo episodic spin-up events known as glitches. If unmodelled by a search, these can result in missed or misidentified detections. We outline a semicoherent glitch-robust search method that allows identification of glitching signal candidates and inference about the model parameters.
9 pages, 6 figures, 2 tables