A semicoherent glitch-robust continuous gravitational wave search

Ashton, Gregory; Prix, Reinhard; Jones, Ian

doi:10.1103/PhysRevD.98.063011

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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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フルテキスト (公開)

1805.03314.pdf
(プレプリント), 2MB

PRD98.063011.pdf
(出版社版), 2MB

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引用

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

引用: https://hdl.handle.net/21.11116/0000-0001-74F5-8

要旨

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.