F. d. M. Blaszczyk

Solar neutrino measurements using the full data period of Super-Kamiokande-IV

First gadolinium loading to Super-Kamiokande

Searching for Supernova Bursts in Super-Kamiokande IV

Neutron tagging following atmospheric neutrino events in a water Cherenkov detector

Diffuse supernova neutrino background search at Super-Kamiokande

Supernova Model Discrimination with Hyper-Kamiokande

Neutron-antineutron oscillation search using a 0.37 megaton-years exposure of Super-Kamiokande

Volume IV. The DUNE far detector single-phase technology

Supernova Neutrino Burst Detection with the Deep Underground Neutrino Experiment

Search for proton decay via <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:msup><mml:mi>e</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mn>0</mml:mn></mml:msup></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:msup><mml:mi>μ</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mm

Neutrino interaction classification with a convolutional neural network in the DUNE far detector

Calorimetry for low-energy electrons using charge and light in liquid argon

Indirect search for dark matter from the Galactic Center and halo with the Super-Kamiokande detector

Deep underground neutrino experiment (DUNE) far detector technical design report

Atmospheric neutrino oscillation analysis with external constraints in Super-Kamiokande I-IV

Measurement of the tau neutrino cross section in atmospheric neutrino oscillations with Super-Kamiokande

Search for Boosted Dark Matter Interacting with Electrons in Super-Kamiokande

Search for nucleon decay into charged antilepton plus meson in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mn>0.316</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mtext>megaton</mml:mtext><mml:mo>·</mml:mo><mml:mtext>years</mml:mtext></mml:mrow></mml:math> exposure of the Super-Kamiokande water Cherenkov detector

Solar neutrino measurements in Super-Kamiokande-IV

Upper bound on neutrino mass based on T2K neutrino timing measurements

Measurements of neutrino oscillation in appearance and disappearance channels by the T2K experiment with<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>6.6</mml:mn><mml:mo>×</mml:mo><mml:mn>1</mml:mn><mml:msup><mml:mn>0</mml:mn><mml:mn>20</mml:mn></mml:msup></mml:math>protons on target

Neutrino oscillation physics potential of the T2K experiment

Measurement of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>ν</mml:mi></mml:mrow><mml:mrow><mml:mi>μ</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math>charged-current quasielastic cross section on carbon with the ND280 detector at T2K

Measurement of the<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:math>charged current quasielastic cross section on carbon with the T2K on-axis neutrino beam

Observation of Electron Neutrino Appearance in a Muon Neutrino Beam

Precise Measurement of the Neutrino Mixing Parameter<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mi>θ</mml:mi><mml:mn>23</mml:mn></mml:msub></mml:math>from Muon Neutrino Disappearance in an Off-Axis Beam

Measurement of the Inclusive Electron Neutrino Charged Current Cross Section on Carbon with the T2K Near Detector

Measurement of the inclusive<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:math>charged current cross section on iron and hydrocarbon in the T2K on-axis neutrino beam

Measurement of the intrinsic electron neutrino component in the T2K neutrino beam with the ND280 detector

Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>γ</mml:mi></mml:mrow></mml:math>rays