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https://hdl.handle.net/2440/137353
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dc.contributor.author | Beniwal, D. | - |
dc.contributor.author | Clearwater, P. | - |
dc.contributor.author | Dunn, L. | - |
dc.contributor.author | Strang, L. | - |
dc.contributor.author | Rowell, G. | - |
dc.contributor.author | Melatos, A. | - |
dc.contributor.author | Ottaway, D. | - |
dc.date.issued | 2022 | - |
dc.identifier.citation | Physical Review D, 2022; 106(10):103018-1-103018-15 | - |
dc.identifier.issn | 2470-0010 | - |
dc.identifier.issn | 2470-0029 | - |
dc.identifier.uri | https://hdl.handle.net/2440/137353 | - |
dc.description | Published 15 November 2022 | - |
dc.description.abstract | We present a search for continuous gravitational-wave signals from an unidentified pulsar potentially poweringHESS J1427-608, a spatially unresolvedTeVpoint source detected by the HighEnergy Stereoscopic System (HESS). The search uses a semicoherent algorithm, which combines the maximum likelihood F statistic with a hidden Markov model to efficiently detect and track quasimonochromatic signals that wander randomly in frequency. It uses data from the second observing run of the Advanced Laser Interferometer Gravitational-Wave Observatory. Multiwavelength observations of the HESS source are combined with the proprieties of the population of TeV-bright pulsar wind nebulae to constrain the search parameters.We find no evidence of gravitational-wave emission from this target.We set upper limits on the characteristic wave strain h95% 0 (for circularly polarized signals) at95%confidence level in sample subbands and interpolate it to estimate the sensitivity in the full band. We find h95% 0 ¼ 1.3 × 10−25 near 185 Hz. The implied constraints on the ellipticity and r-mode amplitude reach ϵ ≤ 10−5 and α ≤ 10−3 at 200 Hz, respectively. | - |
dc.description.statementofresponsibility | Deeksha Beniwal, Patrick Clearwater, Liam Dunn, Lucy Strang, Gavin Rowell, Andrew Melatos, and David Ottaway | - |
dc.language.iso | en | - |
dc.publisher | American Physical Society | - |
dc.rights | © 2022 American Physical Society | - |
dc.source.uri | http://dx.doi.org/10.1103/physrevd.106.103018 | - |
dc.title | Search for continuous gravitational waves from HESS J1427-608 with a hidden Markov model | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1103/physrevd.106.103018 | - |
dc.relation.grant | http://purl.org/au-research/grants/arc/CE170100004 | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Rowell, G. [0000-0002-9516-1581] | - |
dc.identifier.orcid | Ottaway, D. [0000-0001-6794-1591] | - |
Appears in Collections: | IPAS publications Physics publications |
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