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All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

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dc.contributor.authorAbbott, Benjamin P.
dc.contributor.authorAbbott, Richard
dc.contributor.authorAbbott, T.
dc.contributor.authorAbraham, S.
dc.contributor.authorAcernese, F.
dc.contributor.authorAckley, K.
dc.contributor.authorAdams, Catherine Anne
dc.contributor.authorAdhikari, Rana
dc.contributor.authorAdya, V.
dc.contributor.authorAffeldt, C.
dc.contributor.authorAltin, Paul
dc.contributor.authorForsyth, Perry
dc.contributor.authorKijbunchoo, Nutsinee
dc.contributor.authorManske, Michael
dc.contributor.authorMcClelland, David
dc.contributor.authorMcManus, David
dc.contributor.authorMcRae, Terry
dc.contributor.authorScott, Susan M.
dc.contributor.authorShaddock, Daniel
dc.contributor.authorSlagmolen, Bram
dc.contributor.authorWard, Robert
dc.contributor.authorWette, Karl
dc.contributor.authorYap, Min Jet
dc.contributor.authorHolland, Nathan
dc.date.accessioned2020-06-16T01:11:05Z
dc.date.available2020-06-16T01:11:05Z
dc.date.issued2019-07-15
dc.date.updated2021-11-28T07:30:07Z
dc.description.abstractWe present results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast spinning neutron stars with an asymmetry around their rotation axis, using data from the second observing run of the Advanced LIGO detectors. Three different semicoherent methods are used to search in a gravitational-wave frequency band from 20 to 1922 Hz and a first frequency derivative from −1 × 10−8 to 2 × 10−9 Hz=s. None of these searches has found clear evidence for a CW signal, so upper limits on the gravitational-wave strain amplitude are calculated, which for this broad range in parameter space are the most sensitive ever achieved.
dc.description.sponsorshipThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the SpanishAgenciaEstatal de Investigación,the Vicepresid`encia i Conselleria d’Innovació, Recerca i Turisme and the Conselleria d’Educació i Universitat del Govern de les Illes Balears, the Conselleria d’Educació, Investigació, Cultura i Esport de la Generalitat Valenciana, the National Science Centre of Poland, the Swiss National Science Foundation (SNSF), the Russian Foundation for Basic Research, the Russian Science Foundation, the European Commission, the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the Paris Île-de-France Region, the National Research, Development and Innovation Office Hungary (NKFIH), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, the Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, Innovations, and Communications, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS, INFN-CNAF, PLGrid, and the State of Niedersachsen/Germany for provision of computational resources. Work at SURFsara and Nikhef has been performed using resources of the Dutch eInfrastructure, which is financially supported by the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (Netherlands Organisation for Scientific Research, NWO) and the Dutch higher education and research partnership for network services and information and communication technology (SURF).en_AU
dc.format.extent27 pages
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0556-2821en_AU
dc.identifier.urihttp://hdl.handle.net/1885/205166
dc.language.isoen_AUen_AU
dc.provenancehttp://sherpa.ac.uk/romeo/issn/2470-0010/ Author can archive publisher's version/PDF. On author's personal website, employer's website or institutional repository. Publisher's version/PDF may be used (Sherpa/Romeo as of 16/6/2020)en_AU
dc.publisherAmerican Physical Society
dc.rights© 2019 American Physical Society. B. P. Abbott et al. (LIGO Scientific Collaboration and Virgo Collaboration), All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data, Phys. Rev. D 100, 024004 – Published 8 July 2019, DOI 10.1103/PhysRevD.100.024004
dc.sourcePhysical Review D
dc.subjectgravitational wave sources
dc.subjectgravitational waves
dc.subjectneutron stars and pulsars
dc.subjectgravitational wave detection
dc.titleAll-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2en_AU
local.bibliographicCitation.startpage024004en_AU
local.contributor.affiliationAbbott, Benjamin P, California Institute of Technologyen_AU
local.contributor.affiliationAbbott, Richard, California Institute of Technologyen_AU
local.contributor.affiliationAbbott, T, Louisiana State Universityen_AU
local.contributor.affiliationAbraham, S, Inter-University Centre for Astronomy and Astrophysicsen_AU
local.contributor.affiliationAcernese, F, INFNen_AU
local.contributor.affiliationAckley, K, Monash Universityen_AU
local.contributor.affiliationAdams, Catherine Anne, LIGO Livingston Observatoryen_AU
local.contributor.affiliationAdhikari, Rana, LIGO - California Institute of Technologyen_AU
local.contributor.affiliationAdya, V, Max-Planck-Institut für, Gravitationsphysiken_AU
local.contributor.affiliationAffeldt, C, Max-Planck-Institut für Gravitationsphysiken_AU
local.contributor.affiliationAltin, Paul, College of Science, The Australian National Universityen_AU
local.contributor.affiliationForsyth, Perry, College of Science, The Australian National Universityen_AU
local.contributor.affiliationKijbunchoo, Nutsinee, College of Science, The Australian National Universityen_AU
local.contributor.affiliationManske, Michael, College of Science, The Australian National Universityen_AU
local.contributor.affiliationMcClelland, David, College of Science, The Australian National Universityen_AU
local.contributor.affiliationMcManus, David, College of Science, The Australian National Universityen_AU
local.contributor.affiliationMcRae, Terry, College of Science, The Australian National Universityen_AU
local.contributor.affiliationScott, Susan M, College of Science, The Australian National Universityen_AU
local.contributor.affiliationShaddock, Daniel, College of Science, The Australian National Universityen_AU
local.contributor.affiliationSlagmolen, Bram, College of Science, The Australian National Universityen_AU
local.contributor.affiliationWard, Robert, College of Science, The Australian National Universityen_AU
local.contributor.affiliationWette, Karl, College of Science, The Australian National Universityen_AU
local.contributor.affiliationYap, Min Jet, College of Science, The Australian National Universityen_AU
local.contributor.affiliationHolland, Nathan, College of Science, The Australian National Universityen_AU
local.contributor.authoruidAltin, Paul, u4103634en_AU
local.contributor.authoruidForsyth, Perry, u5024171en_AU
local.contributor.authoruidKijbunchoo, Nutsinee, u6400927en_AU
local.contributor.authoruidManske, Michael, t1728en_AU
local.contributor.authoruidMcClelland, David, u8802403en_AU
local.contributor.authoruidMcManus, David, u4671069en_AU
local.contributor.authoruidMcRae, Terry, u1008768en_AU
local.contributor.authoruidScott, Susan M, u8911327en_AU
local.contributor.authoruidShaddock, Daniel, u9701638en_AU
local.contributor.authoruidSlagmolen, Bram, u9905035en_AU
local.contributor.authoruidWard, Robert, u5088188en_AU
local.contributor.authoruidWette, Karl, u4090078en_AU
local.contributor.authoruidYap, Min Jet, u5021389en_AU
local.contributor.authoruidHolland, Nathan, u5748557en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor020105 - General Relativity and Gravitational Wavesen_AU
local.identifier.absfor020106 - High Energy Astrophysics; Cosmic Raysen_AU
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciencesen_AU
local.identifier.ariespublicationu3102795xPUB4729en_AU
local.identifier.citationvolume100en_AU
local.identifier.doi10.1103/PhysRevD.100.024004en_AU
local.identifier.scopusID2-s2.0-85072684605
local.identifier.thomsonIDWOS:000474376200004
local.publisher.urlhttps://www.aps.org/en_AU
local.type.statusPublished Versionen_AU

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