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Sensitivity Studies for Third-Generation Gravitational Wave Observatories
S. Hild, M. Abernathy, F. Acernese +136
Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a…
Phenomenological gravitational waveforms from spinning coalescing binaries
R. Sturani, S. Fischetti, L. Cadonati +4
An accurate knowledge of the coalescing binary gravitational waveform is crucial for experimental searches as the ones performed by the LIGO-Virgo collaboration. Following an earli…
Calibration and sensitivity of the Virgo detector during its second science run
The Virgo Collaboration, T. Accadia, F. Acernese +175
The Virgo detector is a kilometer-length interferometer for gravitational wave detection located near Pisa (Italy). During its second science run (VSR2) in 2009, six months of data…
Complete phenomenological gravitational waveforms from spinning coalescing binaries
R. Sturani, S. Fischetti, L. Cadonati +4
The quest for gravitational waves from coalescing binaries is customarily performed by the LIGO-Virgo collaboration via matched filtering, which requires a detailed knowledge of th…
Virgo calibration and reconstruction of the gravitational wave strain during VSR1
The Virgo collaboration, T. Accadia, F. Acernese +171
Virgo is a kilometer-length interferometer for gravitational waves detection located near Pisa. Its first science run, VSR1, occured from May to October 2007. The aims of the calib…