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805 results on '"Lamoureux, M"'

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201. Measurements of ν̅μ and ν̅μ + νμ charged-current cross-sections without detected pions or protons on water and hydrocarbon at a mean anti-neutrino energy of 0.86 GeV

202. Measurements of ν̅ μ and ν̅ μ + ν μ charged-current cross-sections without detected pions or protons on water and hydrocarbon at a mean anti-neutrino energy of 0.86 GeV

203. Search for tens of MeV neutrinos associated with gamma-ray bursts in Super-Kamiokande

204. Supernova Model Discrimination with Hyper-Kamiokande

205. Measurements of (nu)over-bar(mu) and (nu)over-bar(mu) + nu(mu) charged-current cross-sections without detected pions or protons on water and hydrocarbon at a mean anti-neutrino energy of 0.86 GeV

206. T2K measurements of muon neutrino and antineutrino disappearance using 3.13 x 10(21) protons on target

207. Improved constraints on neutrino mixing from the T2K experiment with $\mathbf{3.13\times10^{21}}$ protons on target

208. Measurements of ν̄μ and ν̄μ + νμ charged-current cross-sections without detected pions nor protons on water and hydrocarbon at mean antineutrino energy of 0.86 GeV

209. Improved constraints on neutrino mixing from the T2K experiment with 3.13 × 10 21 protons on target

210. Improved constraints on neutrino mixing from the T2K experiment with 3.13 × 10 21 protons on target

211. KM3NeT/ARCA sensitivity to transient neutrino sources

212. Measurements of $\overline{\nu}_{\mu}$ and $\overline{\nu}_{\mu} + \nu_{\mu}$ charged-current cross-sections without detected pions or protons on water and hydrocarbon at a mean anti-neutrino energy of 0.86 GeV

213. First T2K measurement of transverse kinematic imbalance in the muon-neutrino charged-current single- production channel containing at least one proton

214. New Methods and Simulations for Cosmogenic Induced Spallation Removal in Super-Kamiokande-IV

215. Nanobeacon: A time calibration device for the KM3NeT neutrino telescope

216. Implementation and first results of the KM3NeT real-time core-collapse supernova neutrino search

217. First Gadolinium Loading to Super-Kamiokande

218. Combined sensitivity of JUNO and KM3NeT/ORCA to the neutrino mass ordering

219. Diffuse Supernova Neutrino Background Search at Super-Kamiokande

220. Sensitivity of the Upgraded T2K Near Detector to constrain neutrino and anti-neutrino interactions with no mesons in the final state by exploiting nucleon-lepton correlations

221. Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA

222. Determining the Neutrino Mass Ordering and Oscillation Parameters with KM3NeT/ORCA

223. Search for neutrinos in coincidence with gravitational wave events from the LIGO-Virgo O3a Observing Run with the Super-Kamiokande detector

224. Improved constraints on neutrino mixing from the T2K experiment with $\mathbf{3.13\times10^{21}}$ protons on target

225. Search for Tens of MeV Neutrinos associated with Gamma-Ray Bursts in Super-Kamiokande

226. First T2K measurement of transverse kinematic imbalance in the muon-neutrino charged-current single-$\pi^+$ production channel containing at least one proton

227. SNEWS 2.0 : a next-generation supernova early warning system for multi-messenger astronomy

228. The KM3NeT potential for the next core-collapse supernova observation with neutrinos

229. Collaborative Experience between Scientific Software Projects using Agile Scrum Development

230. Supernova Model Discrimination with Hyper-Kamiokande

231. SNEWS 2.0:a next-generation supernova early warning system for multi-messenger astronomy

232. Characterization of resistive Micromegas detectors for the upgrade of the T2K Near Detector Time Projection Chambers

233. Search for proton decay via <math><mi>p</mi><mo>→</mo><msup><mi>e</mi><mo>+</mo></msup><msup><mi>π</mi><mn>0</mn></msup></math> and <math><mi>p</mi><mo>→</mo><msup><mi>μ</mi><mo>+</mo></msup><msup><mi>π</mi><mn>0</mn></msup></math> with an enlarged fiducial volume in Super-Kamiokande I-IV

234. Search for neutral-current induced single photon production at the ND280 near detector in T2K

235. SNEWS 2.0: a next-generation supernova early warning system for multi-messenger astronomy

236. First measurement of the charged current <math><msub><mover><mi>ν</mi><mo>¯</mo></mover><mi>μ</mi></msub></math> double differential cross section on a water target without pions in the final state

237. Search for proton decay via p→e+π0 and p→μ+π0 with an enlarged fiducial volume in Super-Kamiokande I-IV

238. First measurement of the charged current (nu)over-bar(mu) double differential cross section on a water target without pions in the final state : (The T2K Collaboration)

239. First measurement of the charged current ν ¯ μ double differential cross section on a water target without pions in the final state FIRST MEASUREMENT of the CHARGED CURRENT ... ABE K. et al

240. Search for proton decay via $p\to e^+��^0$ and $p\to ��^+��^0$ with an enlarged fiducial volume in Super-Kamiokande I-IV

241. T2K measurements of muon neutrino and antineutrino disappearance using $3.13\times 10^{21}$ protons on target

242. Indirect Search for Dark Matter from the Galactic Center and Halo with the Super-Kamiokande Detector

243. Measurements of $\bar{\nu}_{\mu}$ and $\bar{\nu}_{\mu} + \nu_{\mu}$ charged-current cross-sections without detected pions nor protons on water and hydrocarbon at mean antineutrino energy of 0.86 GeV

244. Simultaneous measurement of the muon neutrino charged-current cross section on oxygen and carbon without pions in the final state at T2K

245. First combined measurement of the muon neutrino and antineutrino charged-current cross section without pions in the final state at T2K

246. Measurement of the charged-current electron (anti-)neutrino inclusive cross-sections at the T2K off-axis near detector ND280

247. Search for proton decay via $p\to e^+\pi^0$ and $p\to \mu^+\pi^0$ with an enlarged fiducial volume in Super-Kamiokande I-IV

248. SNEWS 2.0: A Next-Generation SuperNova Early Warning System for Multi-messenger Astronomy

249. Neutron-Antineutron Oscillation Search using a 0.37 Megaton$\cdot$Year Exposure of Super-Kamiokande

250. Search for solar electron anti-neutrinos due to spin-flavor precession in the Sun with Super-Kamiokande-IV

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