Progress report on the gravitational wave experiment in Rome
E. Amaldi(Istituto Nazionale di Fisica Nucleare), G. Vannaroni(Roma Tre University), G. V. Pallottino(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), U. Giovanardi(Plasma (Russia)), B. Pavan(Plasma (Russia)), Valeria Ferrari(Marconi University), C. Cosmelli(Istituto Nazionale di Fisica Nucleare), G. Pizzella(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati), M.-K. Fujimoto(National Astronomical Observatory of Japan), V. Iafolla(Institute for Space Astrophysics and Planetology), Sabrina Ugazio(Plasma (Russia)), Franco Ricci(The University of Adelaide), G. Castellano, F. Fuligni, I. Modena(University of Rome Tor Vergata), P. Bonifazi(Ikerbasque), F. Bordøni, S. Frasca(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), P. Rapagnani(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I)
mgm
January 1, 1982
Cited by 0
Related Papers
KAGRA: 2.5 generation interferometric gravitational wave detector
|Tokyo Tech Research Repository (Tokyo Institute of Technology)|2021|480
Long-term operation of the Rome "Explorer" cryogenic gravitational wave detector
|Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields|1993|155
The Japanese space gravitational wave antenna; DECIGO
|Journal of Physics Conference Series|2008|154
The gravitational wave detector NAUTILUS operating at T = 0.1 K
|Astroparticle Physics|1997|149
Measurement of the VIRGO superattenuator performance for seismic noise suppression
|Review of Scientific Instruments|2001|102