Sensitivity Achieved by the LIGO and Virgo Gravitational Wave Detectors during LIGO's Sixth and Virgo's Second and Third Science Runs

Abstract : We summarize the sensitivity achieved by the LIGO and Virgo gravitational wave detectors for low-mass compact binary coalescence (CBC) searches during LIGO's sixth science run and Virgo's second and third science runs. We present strain noise power spectral densities (PSDs) which are representative of the typical performance achieved by the detectors in these science runs. The data presented here and in the accompanying web-accessible data files are intended to be released to the public as a summary of detector performance for low-mass CBC searches during S6 and VSR2-3.
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Preprints, Working Papers, ...
See paper for full list of authors - Associated data products are publicly accessible here https:.. 2012


http://hal.in2p3.fr/in2p3-00679943
Contributor : Nicole Berger <>
Submitted on : Friday, March 16, 2012 - 4:00:19 PM
Last modification on : Tuesday, October 28, 2014 - 6:00:29 PM

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  • HAL Id : in2p3-00679943, version 1
  • ARXIV : 1203.2674

Citation

J. Abadie, T. Accadia, M. Barsuglia, M. Bebronne, A. Belletoile, et al.. Sensitivity Achieved by the LIGO and Virgo Gravitational Wave Detectors during LIGO's Sixth and Virgo's Second and Third Science Runs. See paper for full list of authors - Associated data products are publicly accessible here https:.. 2012. <in2p3-00679943>

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