Comprehensive all-sky search for periodic gravitational waves in the sixth science run LIGO data

dc.contributorCalifornia Institute of Technology
dc.contributorLouisiana State University
dc.contributorAmerican University
dc.contributorUniversità di Salerno
dc.contributorComplesso Universitario di Monte S.Angelo
dc.contributorUniversity of Florida
dc.contributorLIGO Livingston Observatory
dc.contributorCNRS/IN2P3
dc.contributorUniversity of Sannio at Benevento
dc.contributorMax-Planck-Institut für Gravitationsphysik
dc.contributorScience Park
dc.contributorMassachusetts Institute of Technology
dc.contributorInstituto Nacional de Pesquisas Espaciais
dc.contributorGran Sasso Science Institute
dc.contributorSezione di Roma Tor Vergata
dc.contributorInter-University Centre for Astronomy and Astrophysics
dc.contributorTata Institute of Fundamental Research
dc.contributorUniversity of Wisconsin-Milwaukee
dc.contributorLeibniz Universität Hannover
dc.contributorUniversità di Pisa
dc.contributorSezione di Pisa
dc.contributorAustralian National University
dc.contributorUniversity of Mississippi
dc.contributorCalifornia State University Fullerton
dc.contributorUniversité Paris-Saclay
dc.contributorChennai Mathematical Institute
dc.contributorUniversità di Roma Tor Vergata
dc.contributorUniversity of Southampton
dc.contributorUniversität Hamburg
dc.contributorSezione di Roma
dc.contributorSorbonne Paris Cité
dc.contributorMontana State University
dc.contributorUniversità di Perugia
dc.contributorSezione di Perugia
dc.contributorEuropean Gravitational Observatory (EGO)
dc.contributorSyracuse University
dc.contributorUniversity of Glasgow
dc.contributorLIGO Hanford Observatory
dc.contributorRMKI
dc.contributorColumbia University
dc.contributorStanford University
dc.contributorDipartimento di Fisica e Astronomia
dc.contributorSezione di Padova
dc.contributorCAMK-PAN
dc.contributorUniversity of Birmingham
dc.contributorUniversità degli Studi di Genova
dc.contributorSezione di Genova
dc.contributorRRCAT
dc.contributorLomonosov Moscow State University
dc.contributorUniversity of the West of Scotland
dc.contributorUniversity of Western Australia
dc.contributorRadboud University Nijmegen
dc.contributorObservatoire Côte d'Azur
dc.contributorUniversité de Rennes 1
dc.contributorWashington State University
dc.contributorUniversità degli Studi di Urbino Carlo Bo
dc.contributorSezione di Firenze
dc.contributorUniversity of Oregon
dc.contributorCollège de France
dc.contributorCarleton College
dc.contributorAstronomical Observatory Warsaw University
dc.contributorVU University Amsterdam
dc.contributorUniversity of Maryland
dc.contributorGeorgia Institute of Technology
dc.contributorUniversité Claude Bernard Lyon 1
dc.contributorComplesso Universitario di Monte S. Angelo
dc.contributorNASA/Goddard Space Flight Center
dc.contributorUniversity of Tokyo
dc.contributorTsinghua University
dc.contributorTexas Tech University
dc.contributorNational Tsing Hua University
dc.contributorCharles Sturt University
dc.contributorWest Virginia University
dc.contributorUniversity of Chicago
dc.contributorCaltech CaRT
dc.contributorKorea Institute of Science and Technology Information
dc.contributorUniversità di Roma la Sapienza
dc.contributorUniversity of Brussels
dc.contributorSonoma State University
dc.contributorNorthwestern University
dc.contributorUniversity of Minnesota
dc.contributorUniversity of Melbourne
dc.contributorInstitute for Plasma Research
dc.contributorUniversity of Sheffield
dc.contributorUniversity of Texas Rio Grande Valley
dc.contributorDipartimento di Fisica
dc.contributorTrento Institute for Fundamental Physics and Applications
dc.contributorPennsylvania State University
dc.contributorCardiff University
dc.contributorMontclair State University
dc.contributorLendulet Astrophysics Research Group
dc.contributorNational Astronomical Observatory of Japan
dc.contributorUniversity of Edinburgh
dc.contributorIndian Institute of Technology
dc.contributorUniversity of Szeged
dc.contributorEmbry-Riddle Aeronautical University
dc.contributorOsservatorio Astronomico di Capodimonte
dc.contributorUniversity of Michigan
dc.contributorRochester Institute of Technology
dc.contributorUniversity of Illinois at Urbana-Champaign
dc.contributorIEEC
dc.contributorUniversity of Białystok
dc.contributorUniversity of Strathclyde
dc.contributorCET Campus
dc.contributorUniversity of Toronto
dc.contributorInstitute of Applied Physics
dc.contributorPusan National University
dc.contributorHanyang University
dc.contributorUniversity of Adelaide
dc.contributorNCBJ
dc.contributorIM-PAN
dc.contributorMonash University
dc.contributorSeoul National University
dc.contributorChinese University of Hong Kong
dc.contributorUniversity of Alabama in Huntsville
dc.contributorUniversity of Massachusetts-Amherst
dc.contributorCNRS
dc.contributorSouthern University and AandM College
dc.contributorCollege of William and Mary
dc.contributorUniversidade Estadual Paulista (UNESP)
dc.contributorUniversity of Cambridge
dc.contributorIISER-Kolkata
dc.contributorHSIC
dc.contributorWhitman College
dc.contributorNational Institute for Mathematical Sciences
dc.contributorUniversité de Lyon
dc.contributorHobart and William Smith Colleges
dc.contributorUniversity of Zielona Góra
dc.contributorUniversity of London
dc.contributorAndrews University
dc.contributorUniversità di Siena
dc.contributorTrinity University
dc.contributorUniversity of Washington
dc.contributorKenyon College
dc.contributorAbilene Christian University
dc.contributorSezione di Napoli
dc.date.accessioned2022-04-29T07:50:12Z
dc.date.accessioned2022-12-20T02:35:58Z
dc.date.available2022-04-29T07:50:12Z
dc.date.available2022-12-20T02:35:58Z
dc.date.created2022-04-29T07:50:12Z
dc.date.issued2016-08-15
dc.identifierPhysical Review D, v. 94, n. 4, 2016.
dc.identifier2470-0029
dc.identifier2470-0010
dc.identifierhttp://hdl.handle.net/11449/228200
dc.identifier10.1103/PhysRevD.94.042002
dc.identifier2-s2.0-84984918708
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5408335
dc.description.abstractWe report on a comprehensive all-sky search for periodic gravitational waves in the frequency band 100-1500 Hz and with a frequency time derivative in the range of [-1.18,+1.00]×10-8 Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our galaxy. This search uses the data from the initial LIGO sixth science run and covers a larger parameter space with respect to any past search. A Loosely Coherent detection pipeline was applied to follow up weak outliers in both Gaussian (95% recovery rate) and non-Gaussian (75% recovery rate) bands. No gravitational wave signals were observed, and upper limits were placed on their strength. Our smallest upper limit on worst-case (linearly polarized) strain amplitude h0 is 9.7×10-25 near 169 Hz, while at the high end of our frequency range we achieve a worst-case upper limit of 5.5×10-24. Both cases refer to all sky locations and entire range of frequency derivative values.
dc.languageeng
dc.relationPhysical Review D
dc.sourceScopus
dc.titleComprehensive all-sky search for periodic gravitational waves in the sixth science run LIGO data
dc.typeArtículos de revistas


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