activity
20102019
most citedObservation of a first candidate in the OPERA experiment in the CNGS beam

203 citations · 390 across the 6 of their papers we have counts for

collaborators

6 papers

physics.ins-det201958 cited

Fast simulation of muons produced at the SHiP experiment using Generative Adversarial Networks

SHiP Collaboration

This paper presents a fast approach to simulating muons produced in interactions of the SPS proton beams with the target of the SHiP experiment. The SHiP experiment will be able to…

hep-ex201452 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-ex201443 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…

hep-ex201429 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…

hep-ex2010203 cited

Observation of a first candidate in the OPERA experiment in the CNGS beam

N. Agafonova et al.

The OPERA neutrino detector in the underground Gran Sasso Laboratory (LNGS) has been designed to perform the first detection of neutrino oscillations in direct appearance mode thro…

hep-ex20105 cited

Measurement of the atmospheric muon charge ratio with the OPERA detector

OPERA Collaboration, N. Agafonova, A. Anokhina +182

The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio in the TeV energy region. We analyzed 403069 atmospheric mu…