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Astrophysically triggered searches for gravitational waves: status and prospects.
Classical and Quantum Gravity, 25
Art. No. 114051.
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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 gamma-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.
|Additional Information:||© 2008 Institute of Physics and IOP Publishing Limited.
Received 10 January 2008, in final form 25 February 2008. Published 15 May 2008.
The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Council of Scientific and Industrial Research of India, the Spanish Ministerio de Educación y Ciencia, the Conselleria d’Economia, Hisenda i Innovació of the Govern de les Illes Balears, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This paper has LIGO Document Number LIGO-P070142-01-Z.|
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|National Science Foundation||UNSPECIFIED|
|Science and Technology Facilities Council (STFC) (UK)||UNSPECIFIED|
|State of Niedersachsen (Germany)||UNSPECIFIED|
|Istituto Nazionale di Fisica Nucleare (Italy)||UNSPECIFIED|
|Centre National de la Recherche Scientifique||UNSPECIFIED|
|Australian Research Council||UNSPECIFIED|
|Council of Scientific and Industrial Research of India||UNSPECIFIED|
|Ministerio de Educación y Ciencia (Spain)||UNSPECIFIED|
|Hisenda i Innovació of the Govern de les Illes Balears||UNSPECIFIED|
|Scottish Funding Council||UNSPECIFIED|
|Scottish Universities Physics Alliance||UNSPECIFIED|
|David and Lucile Packard Foundation||UNSPECIFIED|
|Alfred P. Sloan Foundation||UNSPECIFIED|
|Subject Keywords:||GAMMA-RAY BURSTS; ACCRETING NEUTRON-STARS; SGR 1806-20; ENERGY NEUTRINOS; 2004 HYPERFLARE; GIANT FLARE; DISCOVERY; OSCILLATIONS; SENSITIVITY; DETECTOR|
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|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited On:||09 Jan 2009 05:17|
|Last Modified:||25 Feb 2014 22:45|
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