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A semicoherent glitch-robust continuous gravitational wave search

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arxiv 1805.03314 v1 pith:WUJHMSQ4 submitted 2018-05-08 gr-qc astro-ph.HE

classification gr-qcastro-ph.HE
keywords searchcontinuousglitch-robustsemicoherentallowscandidatesdetectionsepisodic
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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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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. First fast radio burst search campaign at the Argentine Institute of Radio Astronomy

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    The IAR campaign found one FRB candidate with DM 243 pc cm^-3 and S/N 8.2, backed by successful recovery of archival and injected bursts.

  2. One-stop strategy to search for long-duration gravitational-wave signals

    gr-qc 2024-11 conditional novelty 6.0 of 10

    A generic GPU search engine plus a fast semianalytic sensitivity estimator could make blind continuous gravitational-wave searches much cheaper to run and characterize.

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