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On Valency

published · living versions
W_4wjzqtpm·v1 · currentpublished
Measurement of the neutrino velocity with the OPERA detector in the CNGS beam
with The OPERA Collaboration, T. Adam, N. Agafonova, A. Aleksandrov +186
1 version

Preprints & journals

30 papers in the corpus · 2005–2025
Observation of Collider Neutrinos without Final State Muons with the SND@LHC Experiment.40577722 · Abbaneo, D, Ahmad, S, Albanese, R et al.2025 · 8 citationsPhysical review letters. 2025;134(23):231802
Contribution of the light-collection non-uniformity to the energy resolution for the spaghetti-type calorimeter modules2409.12927v3 · Vasilisa Guliaeva, Sergey Kholodenko, Evgenii Shmanin et al.2024 · 0 citationsarXiv
Observation of Collider Muon Neutrinos with the SND@LHC Experiment.37540851 · Albanese, R, Alexandrov, A, Alicante, F et al.2023 · 66 citationsPhysical review letters. 2023;131(3):031802
Directional Sensitivity of the NEWSdm Experiment to Cosmic Ray Boosted Dark Matter2305.00112v4 · N.Y. Agafonova, A. Alexandrov, A.M. Anokhina et al.2023 · 9 citationsarXiv
OPERA tau neutrino charged current interactions.34385471 · Agafonova, N, Alexandrov, A, Anokhina, A et al.2024 · 6 citationsScientific data. 2021;8(1):218
Sensitivity of the SHiP experiment to dark photons decaying to a pair of charged particles2011.05115v2 · C. Ahdida, A. Akmete, R. Albanese et al.2020 · 38 citationsarXiv
SND@LHC2002.08722v1 · C. Ahdida, A. Akmete, R. Albanese et al.2020 · 14 citationsarXiv
Final results on neutrino oscillation parameters from the OPERA experiment in the CNGS beam1904.05686v2 · N. Agafonova, A. Alexandrov, A. Anokhina et al.2019 · 21 citationsPhys. Rev. D 100, 051301 (2019)
Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam1811.00095v2 · N. Agafonova, A. Alexandrov, A. Anokhina et al.2018 · 1 citationarXiv
Final Results of the OPERA Experiment on ν_τ Appearance in the CNGS Neutrino Beam.29883136 · Agafonova, N, Alexandrov, A, Anokhina, A et al.2018 · 113 citationsPhysical review letters. 2018;120(21):211801
Discovery potential for directional Dark Matter detection with nuclear emulsions1705.00613v2 · N. Agafonova, A. Aleksandrov, A. Anokhina et al.2017 · 46 citationsarXiv
NEWS: Nuclear Emulsions for WIMP Search1604.04199v1 · A. Aleksandrov, A. Anokhina, T. Asada et al.2016 · 17 citationsarXiv
Discovery of τ Neutrino Appearance in the CNGS Neutrino Beam with the OPERA Experiment.26430986 · Agafonova, N, Aleksandrov, A, Anokhina, A et al.2015 · 163 citationsPhysical review letters. 2015;115(12):121802
How to deal with PCR composition problem at E0≳1017E_0 \gtrsim 10^{17} eV1507.03150v1 · V.I. Galkin, A.M. Anokhina, R. Bakhromzod et al.2015 · 0 citationsarXiv
Observation of nu_tau appearance in the CNGS beam with the OPERA experiment1407.3513v2 · N. Agafonova, A. Aleksandrov, A. Anokhina et al.2014 · 52 citationsarXiv
Determination of the muon charge sign with the dipolar spectrometers of the OPERA experiment1404.5933v3 · N. Agafonova, A. Aleksandrov, A. Anokhina et al.2014 · 3 citationsarXiv
Measurement of TeV atmospheric muon charge ratio with the full OPERA data1403.0244v1 · N. Agafonova, A. Anokhina, S. Aoki et al.2014 · 27 citationsarXiv
Evidence for νμ→ντ\nu_\mu \to \nu_\tau appearance in the CNGS neutrino beam with the OPERA experiment1401.2079v1 · N. Agafonova, A. Aleksandrov, A. Anokhina et al.2014 · 92 citationsPhys. Rev. D 89, 051102 (2014)
The NESSiE Concept for Sterile Neutrinos1312.1227v1 · L. Stanco, A. Anokhina, A. Bagulya et al.2013 · 2 citationsarXiv
Search for νμ→νe\nu_\mu \rightarrow \nu_e oscillations with the OPERA experiment in the CNGS beam1303.3953v2 · N. Agafonova, A. Aleksandrov, A. Anokhina et al.2013 · 7 citationsJHEP07(2013)004
Measurement of the neutrino velocity with the OPERA detector in the CNGS beam1109.4897v4 · T. Adam, N. Agafonova, A. Aleksandrov et al.2011 · 485 citationsarXivon Valency
Measurement of the atmospheric muon charge ratio with the OPERA detector1003.1907v1 · N. Agafonova, A. Anokhina, S. Aoki et al.2010 · 39 citationsarXiv
Career total: at least 140 works. 30 are in this corpus.

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