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  A semicoherent glitch-robust continuous gravitational wave search

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.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0001-74F5-8 Version Permalink: http://hdl.handle.net/21.11116/0000-0002-E815-1
Genre: Journal Article

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 Creators:
Ashton, Gregory1, Author              
Prix, Reinhard1, Author              
Jones, Ian, Author
Affiliations:
1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE
 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.

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 Dates: 2018-05-082018
 Publication Status: Published in print
 Pages: 9 pages, 6 figures, 2 tables
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 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1805.03314
URI: http://arxiv.org/abs/1805.03314
DOI: 10.1103/PhysRevD.98.063011
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Title: Physical Review D
  Other : Phys. Rev. D.
Source Genre: Journal
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Publ. Info: Lancaster, Pa. : American Physical Society
Pages: - Volume / Issue: 98 Sequence Number: 063011 Start / End Page: - Identifier: ISSN: 0556-2821
CoNE: https://pure.mpg.de/cone/journals/resource/111088197762258