Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/48827
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Type: Journal article
Title: Setting upper limits on the strength of periodic gravitational waves from PSR J1939+2134 using the first science data from the GEO 600 and LIGO detectors
Author: Abbott, B.
Abbott, R.
Adhikari, R.
Ageev, A.
Allen, B.
Amin, R.
Anderson, S.
Anderson, W.
Araya, M.
Armandula, H.
Asiri, F.
Aufmuth, P.
Aulbert, C.
Babak, S.
Balasubramanian, R.
Ballmer, S.
Barish, B.
Barker, C.
Barker, D.
Barnes, M.
et al.
Citation: Physical Review. D. Particles, Fields, Gravitation and Cosmology, 2004; 69(8):082004-1-082004-16
Publisher: American Physical Soc
Issue Date: 2004
ISSN: 1550-7998
2470-0029
Statement of
Responsibility: 
B. Allen...C.J. Killow...C. Kim...D. Ottaway...et al.
Abstract: Data collected by the GEO 600 and LIGO interferometric gravitational wave detectors during their first observational science run were searched for continuous gravitational waves from the pulsar J1939+2134 at twice its rotation frequency. Two independent analysis methods were used and are demonstrated in this paper: a frequency domain method and a time domain method. Both achieve consistent null results, placing new upper limits on the strength of the pulsar’s gravitational wave emission. A model emission mechanism is used to interpret the limits as a constraint on the pulsar’s equatorial ellipticity.
Rights: ©2004 American Physical Society
RMID: 0020083090
DOI: 10.1103/PhysRevD.69.082004
Appears in Collections:Physics publications

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