Final Results of the OPERA Experiment on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mi>ν</mml:mi><mml:mi>τ</mml:mi></mml:msub></mml:math> Appearance in the CNGS Neutrino BeamN. Yu. Agafonova, C. Kamiscioglu, A. Alexandrov et al.|Physical Review Letters|2018Cited by 114
Evidence for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mi>ν</mml:mi><mml:mi>μ</mml:mi></mml:msub><mml:mo>→</mml:mo><mml:msub><mml:mi>ν</mml:mi><mml:mi>τ</mml:mi></mml:msub></mml:math>appearance in the CNGS neutrino beam with the OPERA experimentN. Yu. Agafonova, G. Grella, А. Александров et al.|Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields|2014Cited by 93
Measurement of the TeV atmospheric muon charge ratio with the complete OPERA data setN. Yu. Agafonova, C. Kamiscioglu, C. Bozza et al.|The European Physical Journal C|2014Cited by 29
Final results of the search for νμ → νe oscillations with the OPERA detector in the CNGS beamN. Yu. Agafonova, C. Jollet, A. Iuliano et al.|Journal of High Energy Physics|2018Cited by 27