Phys. Rev. D
80,
042003
(2009)
[14 pages]
Einstein@Home search for periodic gravitational waves in early S5 LIGO data
B. P. Abbott et al. LIGO Scientific Collaboration
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B. P. Abbott17, R. Abbott17, R. Adhikari17, P. Ajith2, B. Allen2,60, G. Allen35, R. S. Amin21, S. B. Anderson17, W. G. Anderson60, M. A. Arain47, M. Araya17, H. Armandula17, P. Armor60, Y. Aso17, S. Aston46, P. Aufmuth16, C. Aulbert2, S. Babak1, P. Baker24, S. Ballmer17, C. Barker18, D. Barker18, B. Barr48, P. Barriga59, L. Barsotti20, M. A. Barton17, I. Bartos10, R. Bassiri48, M. Bastarrika48, B. Behnke1, M. Benacquista42, J. Betzwieser17, P. T. Beyersdorf31, I. A. Bilenko25, G. Billingsley17, R. Biswas60, E. Black17, J. K. Blackburn17, L. Blackburn20, D. Blair59, B. Bland18, T. P. Bodiya20, L. Bogue19, R. Bork17, V. Boschi17, S. Bose61, P. R. Brady60, V. B. Braginsky25, J. E. Brau53, D. O. Bridges19, M. Brinkmann2, A. F. Brooks17, D. A. Brown36, A. Brummit30, G. Brunet20, A. Bullington35, A. Buonanno49, O. Burmeister2, R. L. Byer35, L. Cadonati50, J. B. Camp26, J. Cannizzo26, K. C. Cannon17, J. Cao20, L. Cardenas17, S. Caride51, G. Castaldi56, S. Caudill21, M. Cavaglià39, C. 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1Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany 2Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany 3Andrews University, Berrien Springs, Michigan 49104, USA 4Australian National University, Canberra, 0200, Australia 5California Institute of Technology, Pasadena, California 91125, USA 6Caltech-CaRT, Pasadena, California 91125, USA 7Cardiff University, Cardiff, CF24 3AA, United Kingdom 8Carleton College, Northfield, Minnesota 55057, USA 9Charles Sturt University, Wagga Wagga, NSW 2678, Australia 10Columbia University, New York, New York 10027, USA 11Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA 12Eötvös University, ELTE 1053 Budapest, Hungary 13Hobart and William Smith Colleges, Geneva, New York 14456, USA 14Institute of Applied Physics, Nizhny Novgorod, 603950, Russia 15Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India 16Leibniz Universität Hannover, D-30167 Hannover, Germany 17LIGO–California Institute of Technology, Pasadena, California 91125, USA 18LIGO–Hanford Observatory, Richland, Washington 99352, USA 19LIGO–Livingston Observatory, Livingston, Louisiana 70754, USA 20LIGO–Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA 21Louisiana State University, Baton Rouge, Louisiana 70803, USA 22Louisiana Tech University, Ruston, Louisiana 71272, USA 23Loyola University, New Orleans, Louisiana 70118, USA 24Montana State University, Bozeman, Montana 59717, USA 25Moscow State University, Moscow, 119992, Russia 26NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA 27National Astronomical Observatory of Japan, Tokyo 181-8588, Japan 28Northwestern University, Evanston, Illinois 60208, USA 29Rochester Institute of Technology, Rochester, New York 14623, USA 30Rutherford Appleton Laboratory, HSIC, Chilton, Didcot, Oxon OX11 0QX, United Kingdom 31San Jose State University, San Jose, California 95192, USA 32Sonoma State University, Rohnert Park, California 94928, USA 33Southeastern Louisiana University, Hammond, Louisiana 70402, USA 34Southern University and A&M College, Baton Rouge, Louisiana 70813, USA 35Stanford University, Stanford, California 94305, USA 36Syracuse University, Syracuse, New York 13244, USA 37The Pennsylvania State University, University Park, Pennsylvania 16802, USA 38The University of Melbourne, Parkville VIC 3010, Australia 39The University of Mississippi, University, Mississippi 38677, USA 40The University of Sheffield, Sheffield S10 2TN, United Kingdom 41The University of Texas at Austin, Austin, Texas 78712, USA 42The University of Texas at Brownsville and Texas Southmost College, Brownsville, Texas 78520, USA 43Trinity University, San Antonio, Texas 78212, USA 44Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain 45University of Adelaide, Adelaide, SA 5005, Australia 46University of Birmingham, Birmingham, B15 2TT, United Kingdom 47University of Florida, Gainesville, Florida 32611, USA 48University of Glasgow, Glasgow, G12 8QQ, United Kingdom 49University of Maryland, College Park, Maryland 20742, USA 50University of Massachusetts–Amherst, Amherst, Massachusetts 01003, USA 51University of Michigan, Ann Arbor, Michigan 48109, USA 52University of Minnesota, Minneapolis, Minnesota 55455, USA 53University of Oregon, Eugene, Oregon 97403, USA 54University of Rochester, Rochester, New York 14627, USA 55University of Salerno, 84084 Fisciano (Salerno), Italy 56University of Sannio at Benevento, I-82100 Benevento, Italy 57University of Southampton, Southampton, SO17 1BJ, United Kingdom 58University of Strathclyde, Glasgow, G1 1XQ, United Kingdom 59University of Western Australia, Crawley, Washington 6009, Australia, USA 60University of Wisconsin–Milwaukee, Milwaukee, Wisconsin 53201, USA 61Washington State University, Pullman, Washington 99164, USA
D. P. Anderson
University of California at Berkeley, Berkeley, California 94720, USA
Received 29 May 2009; published 11 August 2009
This paper reports on an all-sky search for periodic gravitational waves from sources such as deformed isolated rapidly spinning neutron stars. The analysis uses 840 hours of data from 66 days of the fifth LIGO science run (S5). The data were searched for quasimonochromatic waves with frequencies f in the range from 50 to 1500 Hz, with a linear frequency drift f˙ (measured at the solar system barycenter) in the range -f/τ<f˙<0.1f/τ, for a minimum spin-down age τ of 1000 years for signals below 400 Hz and 8000 years above 400 Hz. The main computational work of the search was distributed over approximately 100 000 computers volunteered by the general public. This large computing power allowed the use of a relatively long coherent integration time of 30 hours while searching a large parameter space. This search extends Einstein@Home’s previous search in LIGO S4 data to about 3 times better sensitivity. No statistically significant signals were found. In the 125–225 Hz band, more than 90% of sources with dimensionless gravitational-wave strain tensor amplitude greater than 3×10-24 would have been detected.
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Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.
© 2009 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevD.80.042003
DOI:
10.1103/PhysRevD.80.042003
PACS:
04.80.Nn, 95.55.Ym, 97.60.Gb, 07.05.Kf
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