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Search for gravitational waves from five low mass X-ray binaries in the second Advanced LIGO observing run with an improved hidden Markov model

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arxiv 2006.06907 v2 pith:5SQIJB5G submitted 2020-06-12 astro-ph.HE astro-ph.IMgr-qc

classification astro-ph.HEastro-ph.IMgr-qc
keywords searchx-raybinariesfiveobservingadvancedcandidatesgravitational
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Low mass X-ray binaries are prime targets for continuous gravitational wave searches by ground-based interferometers. Results are presented from a search for five low-mass X-ray binaries whose spin frequencies and orbital elements are measured accurately from X-ray pulsations: HETE J1900.1-2455, IGR J00291+5934, SAX J1808.4-3658, XTE J0929-314, and XTE J1814-338. Data are analysed from Observing Run 2 of the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO). The search algorithm uses a hidden Markov model to track spin wandering, the $\mathcal{J}$-statistic maximum likelihood matched filter to track orbital phase, and a suite of five vetoes to reject artefacts from non-Gaussian noise. The search yields a number of low-significance, above threshold candidates consistent with the selected false-alarm probability. The candidates will be followed up in subsequent observing runs.

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Cited by 1 Pith paper

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

  1. Spotlight searches for continuous gravitational waves triggered on radiometer candidates in LIGO O4a data

    gr-qc 2026-08 accept novelty 5.0 of 10

    No continuous gravitational-wave signal was found in any of the 562 radiometer-triggered candidates after vetoes and an O4b follow-up; the search reaches 95% detection efficiency for strains around 0.63 to 6.3 times 10^-25.

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