Authors

J. Aasi, California Institute of TechnologyFollow
J. Abadie, California Institute of TechnologyFollow
B. P. Abbott, California Institute of TechnologyFollow
R. Abbott, California Institute of TechnologyFollow
T. D. Abbott, California State University, FullertonFollow
M. Abernathy, University of GlasgowFollow
T. Accadia, Université Savoie Mont BlancFollow
F. Acernese, Istituto Nazionale di Fisica Nucleare, Sezione di NapoliFollow
C. Adams, LIGO LivingstonFollow
T. Adams, Cardiff UniversityFollow
P. Addesso, Università degli Studi del SannioFollow
R. Adhikari, California Institute of TechnologyFollow
C. Affeldt, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)Follow
M. Agathos, FOM-Institute of Subatomic Physics - NIKHEFFollow
K. Agatsuma, National Institutes of Natural Sciences - National Astronomical Observatory of JapanFollow
P. Ajith, California Institute of TechnologyFollow
B. Allen, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)Follow
A. Allocca, Istituto Nazionale di Fisica Nucleare, Sezione di PisaFollow
E. Amador Ceron, University of Wisconsin-MilwaukeeFollow
D. Amariutei, University of FloridaFollow
S. B. Anderson, California Institute of TechnologyFollow
W. G. Anderson, University of Wisconsin-MilwaukeeFollow
K. Arai, California Institute of Technology
M. C. Araya, California Institute of Technology
S. Ast, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
S. M. Aston, LIGO Livingston
P. Astone, Istituto Nazionale di Fisica Nucleare - INFN
D. Atkinson, LIGO Hanford
P. Aufmuth, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
C. Aulbert, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
B. E. Aylott, University of Birmingham
S. Babak, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
P. Baker, Montana State University

Document Type

Article

Publication Date

2-13-2013

Abstract

This paper presents results of an all-sky search for periodic gravitational waves in the frequency range [50,1 190] Hz and with frequency derivative range of ∼[-20,1.1]×10-10 Hz s-1 for the fifth LIGO science run (S5). The search uses a noncoherent Hough-transform method to combine the information from coherent searches on time scales of about one day. Because these searches are very computationally intensive, they have been carried out with the Einstein@Home volunteer distributed computing project. Postprocessing identifies eight candidate signals; deeper follow-up studies rule them out. Hence, since no gravitational wave signals have been found, we report upper limits on the intrinsic gravitational wave strain amplitude h 0. For example, in the 0.5 Hz-wide band at 152.5 Hz, we can exclude the presence of signals with h0 greater than 7.6×10 -25 at a 90% confidence level. This search is about a factor 3 more sensitive than the previous Einstein@Home search of early S5 LIGO data. © 2013Published by the American Physical Society.

Publication Source (Journal or Book title)

Physical Review D - Particles, Fields, Gravitation and Cosmology

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