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Journal Article

A semicoherent glitch-robust continuous gravitational wave search

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Ashton,  Gregory
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Prix,  Reinhard
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Fulltext (public)

1805.03314.pdf
(Preprint), 2MB

PRD98.063011.pdf
(Publisher version), 2MB

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Citation

Ashton, G., Prix, R., & Jones, I. (2018). A semicoherent glitch-robust continuous gravitational wave search. Physical Review D, 98: 063011. doi:10.1103/PhysRevD.98.063011.


Cite as: http://hdl.handle.net/21.11116/0000-0001-74F5-8
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.