Home > Research > Publications & Outputs > All-Sky LIGO Search for Periodic Gravitational ...

Research

Links

Text available via DOI:

Keywords

View graph of relations

All-Sky LIGO Search for Periodic Gravitational Waves in the Early Fifth-Science-Run Data

Research output: Contribution to Journal/Magazine › Letter › peer-review

Published

Standard

All-Sky LIGO Search for Periodic Gravitational Waves in the Early Fifth-Science-Run Data. / LIGO Scientific Collaboration.

In: Physical review letters, Vol. 102, No. 11, 111102, 20.03.2009.

Research output: Contribution to Journal/Magazine › Letter › peer-review

Harvard

LIGO Scientific Collaboration 2009, 'All-Sky LIGO Search for Periodic Gravitational Waves in the Early Fifth-Science-Run Data', Physical review letters, vol. 102, no. 11, 111102. https://doi.org/10.1103/PhysRevLett.102.111102

APA

LIGO Scientific Collaboration (2009). All-Sky LIGO Search for Periodic Gravitational Waves in the Early Fifth-Science-Run Data. Physical review letters, 102(11), [111102]. https://doi.org/10.1103/PhysRevLett.102.111102

Vancouver

LIGO Scientific Collaboration. All-Sky LIGO Search for Periodic Gravitational Waves in the Early Fifth-Science-Run Data. Physical review letters. 2009 Mar 20;102(11):111102. doi: 10.1103/PhysRevLett.102.111102

Author

LIGO Scientific Collaboration. / All-Sky LIGO Search for Periodic Gravitational Waves in the Early Fifth-Science-Run Data. In: Physical review letters. 2009 ; Vol. 102, No. 11.

Bibtex

@article{b454eec898d443d9a41bc8e9633d1629,
title = "All-Sky LIGO Search for Periodic Gravitational Waves in the Early Fifth-Science-Run Data",
abstract = "We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50–1100 Hz and with the frequency{\textquoteright}s time derivative in the range −5×10−9–0 Hz s−1. Data from the first eight months of the fifth LIGO science run (S5) have been used in this search, which is based on a semicoherent method (PowerFlux) of summing strain power. Observing no evidence of periodic gravitational radiation, we report 95% confidence-level upper limits on radiation emitted by any unknown isolated rotating neutron stars within the search range. Strain limits below 10−24 are obtained over a 200-Hz band, and the sensitivity improvement over previous searches increases the spatial volume sampled by an average factor of about 100 over the entire search band. For a neutron star with nominal equatorial ellipticity of 10−6, the search is sensitive to distances as great as 500 pc.",
keywords = "04.80.Nn, 07.05.Kf, 95.55.Ym, 97.60.Gb, Gravitational wave detectors and experiments, Data analysis: algorithms and implementation, data management, Gravitational radiation detectors, mass spectrometers, and other instrumentation and techniques, Pulsars, General Relativity and Quantum Cosmology, Astrophysics",
author = "{LIGO Scientific Collaboration} and M. Pitkin",
year = "2009",
month = mar,
day = "20",
doi = "10.1103/PhysRevLett.102.111102",
language = "English",
volume = "102",
journal = "Physical review letters",
issn = "1079-7114",
publisher = "American Physical Society",
number = "11",

}

RIS

TY - JOUR

T1 - All-Sky LIGO Search for Periodic Gravitational Waves in the Early Fifth-Science-Run Data

AU - LIGO Scientific Collaboration

AU - Pitkin, M.

PY - 2009/3/20

Y1 - 2009/3/20

N2 - We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50–1100 Hz and with the frequency’s time derivative in the range −5×10−9–0 Hz s−1. Data from the first eight months of the fifth LIGO science run (S5) have been used in this search, which is based on a semicoherent method (PowerFlux) of summing strain power. Observing no evidence of periodic gravitational radiation, we report 95% confidence-level upper limits on radiation emitted by any unknown isolated rotating neutron stars within the search range. Strain limits below 10−24 are obtained over a 200-Hz band, and the sensitivity improvement over previous searches increases the spatial volume sampled by an average factor of about 100 over the entire search band. For a neutron star with nominal equatorial ellipticity of 10−6, the search is sensitive to distances as great as 500 pc.

AB - We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50–1100 Hz and with the frequency’s time derivative in the range −5×10−9–0 Hz s−1. Data from the first eight months of the fifth LIGO science run (S5) have been used in this search, which is based on a semicoherent method (PowerFlux) of summing strain power. Observing no evidence of periodic gravitational radiation, we report 95% confidence-level upper limits on radiation emitted by any unknown isolated rotating neutron stars within the search range. Strain limits below 10−24 are obtained over a 200-Hz band, and the sensitivity improvement over previous searches increases the spatial volume sampled by an average factor of about 100 over the entire search band. For a neutron star with nominal equatorial ellipticity of 10−6, the search is sensitive to distances as great as 500 pc.

KW - 04.80.Nn

KW - 07.05.Kf

KW - 95.55.Ym

KW - 97.60.Gb

KW - Gravitational wave detectors and experiments

KW - Data analysis: algorithms and implementation

KW - data management

KW - Gravitational radiation detectors

KW - mass spectrometers

KW - and other instrumentation and techniques

KW - Pulsars

KW - General Relativity and Quantum Cosmology

KW - Astrophysics

U2 - 10.1103/PhysRevLett.102.111102

DO - 10.1103/PhysRevLett.102.111102

M3 - Letter

VL - 102

JO - Physical review letters

JF - Physical review letters

SN - 1079-7114

IS - 11

M1 - 111102

ER -