The most powerful scintillator supernovae detector: LVDM. Aglietta, G. Landi, P. Giusti et al.|Nuovo cimento della Società italiana di fisica. A, Nuclei, particles and fields|1992Cited by 122
Muon “depth-intensity” relation measured by the LVD underground experiment and cosmic-ray muon spectrum at sea levelM. Aglietta, K. Lau, B. Alpat et al.|Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields|1998Cited by 104
Neutron flux generated by cosmic-ray mouns at 5200 hg/cm2 s.r. underground. Depth-neutron intensity curveM. Aglietta, Г. Т. Зацепин, G. Badino et al.|Il Nuovo Cimento C|1989Cited by 54
Limits on low-energy neutrino fluxes with the Mont Blanc liquid scintillator detectorM. Aglietta, Г. Т. Зацепин, P. Antonioli et al.|Astroparticle Physics|1992Cited by 36
Coincidences among the data recorded by the baksan, kamioka and mont blanc underground neutrino detectors, and by the Maryland and Rome gravitational-wave detectors during Supernova 1987 AM. Aglietta, G. Wilmot, A. Castellina et al.|Il Nuovo Cimento C|1991Cited by 27