Time dispersion and efficiency of coincident detection of signals in resonant bar gravitational wave detectors

P. Astone, S. D’Antonio, and G. Pizzella
Phys. Rev. D 62, 042001 – Published 30 June 2000
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Abstract

Using simulated signals and measured noise with the EXPLORER and NAUTILUS detectors we find the efficiency of signal detection and the signal arrival time dispersion versus the signal-to-noise ratio.

  • Received 28 January 2000

DOI:https://doi.org/10.1103/PhysRevD.62.042001

©2000 American Physical Society

Authors & Affiliations

P. Astone, S. D’Antonio, and G. Pizzella

  • University of Rome Tor Vergata, INFN, Sezione di Roma, Rome, Italy
  • INFN, Laboratori Nazionali di Frascati, P.O. Box 13, I-00044 Frascati, Italy

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Issue

Vol. 62, Iss. 4 — 15 August 2000

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