BP
B. D. Park
hep-exphysics.ins-dethep-phastro-ph.COBrain NeoplasmsCranial IrradiationHippocampusHyperArcRadiotherapy DosageRadiotherapy, Intensity-Modulated
On Valency
published · living versionsW_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
19 papers in the corpus · 2011–2024Probing the mixing between sterile and tau neutrinos in the SHiP experiment2403.04191v2 · Ki-Young Choi, Sung Hyun Kim, Yeong Gyun Kim et al.2024 · 2 citationsJ. High Energ. Phys. 2024, 166 (2024)
Dosimetric comparison between RapidArc and HyperArc in hippocampal-sparing whole-brain radiotherapy with a simultaneous integrated boost.37718172 · Kim, Jeongho, Kim, Tae Gyu, Park, Byungdo et al.2024 · 5 citationsMedical dosimetry : official journal of the American Association of Medical Dosimetrists. 2024;49(2):69-76
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
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
Final results of the search for oscillations with the OPERA detector in the CNGS beam1803.11400v2 · N. Agafonova, A. Aleksandrov, A. Anokhina et al.2018 · 30 citationsarXiv
Discovery potential for directional Dark Matter detection with nuclear emulsions1705.00613v2 · N. Agafonova, A. Aleksandrov, A. Anokhina et al.2017 · 46 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
Limits on muon-neutrino to tau-neutrino oscillations induced by a sterile neutrino state obtained by OPERA at the CNGS beam1503.01876v2 · N. Agafonova, A. Aleksandrov, A. Anokhina et al.2015 · 29 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
Procedure for short-lived particle detection in the OPERA experiment and its application to charm decays1404.4357v1 · N. Agafonova, A. Anokhina, S. Aoki et al.2014 · 43 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 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)
Measurement of the neutrino velocity with the OPERA detector in the CNGS beam using the 2012 dedicated data1212.1276v2 · T. Adam, N. Agafonova, A. Aleksandrov et al.2012 · 49 citationsarXiv
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
Career total: at least 68 works. 19 are in this corpus.
Profile built from the corpus for this byline.
Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.