Upper limit at 1.8 kHz for a gravitational-wave stochastic background with the it ALTAIR resonant-mass detector
P. Astone(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), M. Visco(Istituto Nazionale di Fisica Nucleare), G. Pizzella(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati), R. Terenzi, Arturo Moleti(University of Rome Tor Vergata), P. Modestino, M. Bassan(University of Rome Tor Vergata), I. Modena(University of Rome Tor Vergata), P. Bonifazi(Ikerbasque), V. Fafone(University of Rome Tor Vergata), S. Frasca(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), Y. Minenkov(University of Rome Tor Vergata), E. Coccia(University of Rome Tor Vergata), P. Carelli(Istituto Nazionale di Fisica Nucleare), G. V. Pallottino(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I)
Unknown
March 1, 1999
Cited by 6
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