activity
20002026
most citedObservation of a narrow charmonium-like state in exclusive B+ -> K+ pi+pi- J/psi decays

2k citations · 12.7k across the 131 of their papers we have counts for

collaborators
Showing 2014Show all

7 papers · 1 filter

physics.ins-det2014★ 6 cited

Solar neutrino with Borexino: results and perspectives

O. Smirnov, G. Bellini, J. Benziger +87

Borexino is a unique detector able to perform measurement of solar neutrinos fluxes in the energy region around 1 MeV or below due to its low level of radioactive background. It wa…

hep-ex2014★ 52 cited

Observation of nu_tau appearance in the CNGS beam with the OPERA experiment

OPERA Collaboration, N. Agafonova, A. Aleksandrov +145

The OPERA experiment is searching for nu_mu -> nu_tau oscillations in appearance mode i.e. via the direct detection of tau leptons in nu_tau charged current interactions. The evide…

hep-ex2014★ 3 cited

Recent Borexino results and prospects for the near future

D. D'Angelo, G. Bellini, J. Benziger +85

The Borexino experiment, located in the Gran Sasso National Laboratory, is an organic liquid scintillator detector conceived for the real time spectroscopy of low energy solar neut…

hep-ex2014★ 43 cited

Procedure for short-lived particle detection in the OPERA experiment and its application to charm decays

N. Agafonova, A. Anokhina, S. Aoki +135

The OPERA experiment, designed to perform the first observation of oscillations in appearance mode through the detection of the leptons produced in c…

physics.ins-det2014★ 1 cited

Determination of the muon charge sign with the dipolar spectrometers of the OPERA experiment

OPERA Collaboration, N. Agafonova, A. Aleksandrov +141

The OPERA long-baseline neutrino-oscillation experiment has observed the direct appearance of in the CNGS beam. Two large muon magnetic spectrometers are used to identi…

hep-ex2014★ 29 cited

Measurement of TeV atmospheric muon charge ratio with the full OPERA data

N. Agafonova, A. Anokhina, S. Aoki +134

The OPERA detector, designed to search for oscillations in the CNGS beam, is located in the underground Gran Sasso laboratory, a privileged location to study TeV-scal…