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We summarize the sensitivity achieved by the LIGO and Virgo gravitationalwave detectors for low-mass compact binary coalescence (CBC) searches duringLIGO's sixth science run and Virgo's second and third science runs. We presentstrain noise power spectral densities (PSDs) which are representative of thetypical performance achieved by the detectors in these science runs. The datapresented here and in the accompanying web-accessible data files are intendedto be released to the public as a summary of detector performance for low-massCBC searches during S6 and VSR2-3.

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