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Sensitivity Achieved by the LIGO and Virgo Gravitational Wave Detectors during LIGO's Sixth and Virgo's Second and Third Science Runs
J. Abadie, T. Accadia1, M. Barsuglia2, M. Bebronne1, A. Belletoile1, B. Bouhou2, D. Buskulic1, C. Buy2, E. Chassande-Mottin2, A. Dietz1, M. Granata2, R. Gouaty1, N. Letendre1, F. Marion1, A. Masserot1, B. Mours1, L. Rolland1, E. Tournefier1, D. Verkindt1, M. Yvert1, R. Bonnand3, R. Flaminio3, J. Franc3, M. Galimberti3, C. Michel3, N. Morgado3, L. Pinard3, B. Sassolas3, M.-A. Bizouard4, V. Brisson4, F. Cavalier4, M. Davier4, P. Hello4, N. Leroy4, F. Robinet4, M. Vavoulidis4, R.L. Ward2, M. Was4
For the LIGO, VIRGO collaboration(s)

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.
1:  LAPP - Laboratoire d'Annecy le Vieux de Physique des Particules
2:  APC - UMR 7164 - AstroParticule et Cosmologie
3:  LMA - Laboratoire des matériaux avancés
4:  LAL - Laboratoire de l'Accélérateur Linéaire
APC - Cosmologie et Gravitation
Physics/General Relativity and Quantum Cosmology
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