The cumulative normalized range and its two-curve difference make it easier to see which frequency bands actually limit a gravitational-wave detector's inspiral range.
Sensitivity to Gravitational Waves from Compact Binary Coalescences Achieved during LIGO's Fifth and Virgo's First Science Run
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abstract
We summarize the sensitivity achieved by the LIGO and Virgo gravitational wave detectors for compact binary coalescence (CBC) searches during LIGO's fifth science run and Virgo's first science run. We present noise spectral density curves for each of the four detectors that operated during these science runs which are representative of the typical performance achieved by the detectors for CBC searches. These spectra are intended for release to the public as a summary of detector performance for CBC searches during these science runs.
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Guiding interferometer improvements with the frequency-dependent inspiral range
The cumulative normalized range and its two-curve difference make it easier to see which frequency bands actually limit a gravitational-wave detector's inspiral range.