### Abstract

Original language | English |
---|---|

Pages (from-to) | 671-676 |

Number of pages | 6 |

Journal | Classical and Quantum Gravity |

Volume | 21 |

Issue number | 5 |

Publication status | Published - 2004 |

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*Classical and Quantum Gravity*,

*21*(5), 671-676.

}

*Classical and Quantum Gravity*, vol. 21, no. 5, pp. 671-676.

**Upper limits on the strength of periodic gravitational waves from PSR J1939+2134.** / Allen, B; Abbott, R; Adhikari, R; Amin, R; Anderson, SB; Anderson, WG; Araya, M; Armandula, H; Asiri, F; Aufmuth, P; Aulbert, C; Babak, S; Balasubramanian, R; Ballmer, S; Charlton, Philip.

Research output: Contribution to journal › Article

TY - JOUR

T1 - Upper limits on the strength of periodic gravitational waves from PSR J1939+2134

AU - Allen, B

AU - Abbott, R

AU - Adhikari, R

AU - Amin, R

AU - Anderson, SB

AU - Anderson, WG

AU - Araya, M

AU - Armandula, H

AU - Asiri, F

AU - Aufmuth, P

AU - Aulbert, C

AU - Babak, S

AU - Balasubramanian, R

AU - Ballmer, S

AU - Charlton, Philip

N1 - Imported on 12 Apr 2017 - DigiTool details were: Journal title (773t) = Classical and Quantum Gravity. ISSNs: 0264-9381;

PY - 2004

Y1 - 2004

N2 - The first science run of the LIGO and GEO gravitational wave detectors presented the opportunity to test methods of searching for gravitational waves from known pulsars. Here we present new direct upper limits on the strength of waves from the pulsar PSR J1939+2134 using two independent analysis methods, one in the frequency domain using frequentist statistics and one in the time domain using Bayesian inference. Both methods show that the strain amplitude at Earth from this pulsar is less than a few times 10'22.

AB - The first science run of the LIGO and GEO gravitational wave detectors presented the opportunity to test methods of searching for gravitational waves from known pulsars. Here we present new direct upper limits on the strength of waves from the pulsar PSR J1939+2134 using two independent analysis methods, one in the frequency domain using frequentist statistics and one in the time domain using Bayesian inference. Both methods show that the strain amplitude at Earth from this pulsar is less than a few times 10'22.

KW - Gravitational waves

M3 - Article

VL - 21

SP - 671

EP - 676

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

SN - 0264-9381

IS - 5

ER -