### Abstract

Language | English |
---|---|

Pages | S671-S676 |

Number of pages | 6 |

Journal | Classical and Quantum Gravity |

Volume | 21 |

Issue number | 5 |

DOIs | |

Publication status | Published - 9 Feb 2004 |

### Fingerprint

### Keywords

- LIGO
- geo 600 data
- gravitational wave detectors

### Cite this

*Classical and Quantum Gravity*,

*21*(5), S671-S676. https://doi.org/10.1088/0264-9381/21/5/042

}

*Classical and Quantum Gravity*, vol. 21, no. 5, pp. S671-S676. https://doi.org/10.1088/0264-9381/21/5/042

**Upper limits on the strength of periodic gravitational waves from PSR J1939+2134.** / Allen, B.; Woan, G.; Cantley, C. A.; LIGO Scientific Collaboration.

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 - Woan, G.

AU - Cantley, C. A.

AU - LIGO Scientific Collaboration

N1 - This research paper was authored by multiple individuals. Please consult manuscript for full attribution details.

PY - 2004/2/9

Y1 - 2004/2/9

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 - LIGO

KW - geo 600 data

KW - gravitational wave detectors

U2 - 10.1088/0264-9381/21/5/042

DO - 10.1088/0264-9381/21/5/042

M3 - Article

VL - 21

SP - S671-S676

JO - Classical and Quantum Gravity

T2 - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

SN - 0264-9381

IS - 5

ER -