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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…
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…
A laser gyroscope system to detect the Gravito-Magnetic effect on Earth
A. Di Virgilio, K. U. Schreiber, A. Gebauer +5
Large scale square ring laser gyros with a length of four meters on each side are approaching a sensitivity of 1x10^-11 rad/s/sqrt(Hz). This is about the regime required to measure…
Beam test calibration of the balloon-borne imaging calorimeter for the CREAM experiment
P. S. Marrocchesi, H. S. Ahn, M. G. Bagliesi +22
CREAM (Cosmic Ray Energetics And Mass) is a multi-flight balloon mission designed to collect direct data on the elemental composition and individual energy spectra of cosmic rays.…
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…
Rotational sensitivity of the "G-Pisa" gyrolaser
Jacopo Belfi, Nicolò Beverini, Filippo Bosi +4
G-Pisa is an experiment investigating the possibility to operate a high sensitivity laser gyroscope with area less than for improving the performances of the mirrors su…