Observational performance is described in a gravitational wave detector, indicating advanced sensitivity metrics.
The ultracryogenic resonant-mass gravitational wave (GW) detector NAUTILUS of the Rome group is in continuos operation at the Frascati INFN National Laboratories since December 1995. The detector is cooled at about 0.1 K. The measured spectral amplitude sensitivity is h≅6*10^-22 Hz^-1/2, with a bandwidth of about 1 Hz, and the best pulse sensitivity is of the order of h≅4*10^-19. We describe the detector performances, the search for monochromatic wave and the first experiment of cross-correlation between the data obtained with NAUTILUS and Explorer, the detector of the Rome group located at CERN.
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P. et al. (1998) studied this question.
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