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Astrophysically triggered searches for gravitational wave: status and prospects

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Astrophysically triggered searches for gravitational wave: status and prospects. / LIGO Scientific Collaboration and Virgo Collaboration.
In: Classical and Quantum Gravity, Vol. 25, No. 11, 114051, 15.05.2008.

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

Harvard

LIGO Scientific Collaboration and Virgo Collaboration 2008, 'Astrophysically triggered searches for gravitational wave: status and prospects', Classical and Quantum Gravity, vol. 25, no. 11, 114051. https://doi.org/10.1088/0264-9381/25/11/114051

APA

LIGO Scientific Collaboration and Virgo Collaboration (2008). Astrophysically triggered searches for gravitational wave: status and prospects. Classical and Quantum Gravity, 25(11), Article 114051. https://doi.org/10.1088/0264-9381/25/11/114051

Vancouver

LIGO Scientific Collaboration and Virgo Collaboration. Astrophysically triggered searches for gravitational wave: status and prospects. Classical and Quantum Gravity. 2008 May 15;25(11):114051. doi: 10.1088/0264-9381/25/11/114051

Author

LIGO Scientific Collaboration and Virgo Collaboration. / Astrophysically triggered searches for gravitational wave : status and prospects. In: Classical and Quantum Gravity. 2008 ; Vol. 25, No. 11.

Bibtex

@article{52543ceac9a84e679797b64cf3f244bb,
title = "Astrophysically triggered searches for gravitational wave: status and prospects",
abstract = "In gravitational-wave detection, special emphasis is put onto searches that focus on cosmic events detected by other types of astrophysical observatories. The astrophysical triggers, e.g. from γ-ray and x-ray satellites, optical telescopes and neutrino observatories, provide a trigger time for analyzing gravitational-wave data coincident with the event. In certain cases the expected frequency range, source energetics, directional and progenitor information are also available. Beyond allowing the recognition of gravitational waveforms with amplitudes closer to the noise floor of the detector, these triggered searches should also lead to rich science results even before the onset of Advanced LIGO. In this paper we provide a broad review of LIGO's astrophysically triggered searches and the sources they target.",
keywords = "General Relativity and Quantum Cosmology",
author = "{LIGO Scientific Collaboration and Virgo Collaboration} and M. Pitkin",
year = "2008",
month = may,
day = "15",
doi = "10.1088/0264-9381/25/11/114051",
language = "English",
volume = "25",
journal = "Classical and Quantum Gravity",
issn = "0264-9381",
publisher = "IOP Publishing",
number = "11",

}

RIS

TY - JOUR

T1 - Astrophysically triggered searches for gravitational wave

T2 - status and prospects

AU - LIGO Scientific Collaboration and Virgo Collaboration

AU - Pitkin, M.

PY - 2008/5/15

Y1 - 2008/5/15

N2 - In gravitational-wave detection, special emphasis is put onto searches that focus on cosmic events detected by other types of astrophysical observatories. The astrophysical triggers, e.g. from γ-ray and x-ray satellites, optical telescopes and neutrino observatories, provide a trigger time for analyzing gravitational-wave data coincident with the event. In certain cases the expected frequency range, source energetics, directional and progenitor information are also available. Beyond allowing the recognition of gravitational waveforms with amplitudes closer to the noise floor of the detector, these triggered searches should also lead to rich science results even before the onset of Advanced LIGO. In this paper we provide a broad review of LIGO's astrophysically triggered searches and the sources they target.

AB - In gravitational-wave detection, special emphasis is put onto searches that focus on cosmic events detected by other types of astrophysical observatories. The astrophysical triggers, e.g. from γ-ray and x-ray satellites, optical telescopes and neutrino observatories, provide a trigger time for analyzing gravitational-wave data coincident with the event. In certain cases the expected frequency range, source energetics, directional and progenitor information are also available. Beyond allowing the recognition of gravitational waveforms with amplitudes closer to the noise floor of the detector, these triggered searches should also lead to rich science results even before the onset of Advanced LIGO. In this paper we provide a broad review of LIGO's astrophysically triggered searches and the sources they target.

KW - General Relativity and Quantum Cosmology

U2 - 10.1088/0264-9381/25/11/114051

DO - 10.1088/0264-9381/25/11/114051

M3 - Journal article

VL - 25

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

SN - 0264-9381

IS - 11

M1 - 114051

ER -