{"arxiv_id":"astro-ph/0404457","incoming":{"papers":27,"sentences":39,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":3,"sentences":3,"quotes":[{"arxiv_id":"0812.4639","title":"Sensitivity to neutrino mixing parameters with atmospheric neutrinos","url":"/paper/0812.4639","section":"Migration from neutrino to muon","sentence":"We use the CC cross section of Nuance-v3 [ref] and the Honda flux in 3-dimensional scheme [ref] .","intent_p":0.92,"contests_p":null},{"arxiv_id":"0812.4640","title":"A comparison of the sensitivities of the parameters with atmospheric neutrinos for different analysis methods","url":"/paper/0812.4640","section":"The $χ^2$ analysis","sentence":"We use the CC cross section of Nuance-v3 [ref] and the Honda flux of 3-dimensional scheme [ref] .","intent_p":0.87,"contests_p":null},{"arxiv_id":"2305.07291","title":"Impact of errors in the magnetic field measurement on the precision determination of neutrino oscillation parameters at the proposed ICAL detector at INO","url":"/paper/2305.07291","section":"Events generation","sentence":"Charged current (CC) atmospheric neutrino (and anti-neutrino) events were simulated for an exposure of 1000 years at the ICAL detector using the NUANCE neutrino generator [ref] and Honda 3-D fluxes [ref] .","intent_p":0.99,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":10,"sentences":10,"quotes":[{"arxiv_id":"2105.08744","title":"Violation of Equivalence Principle in Neutrino Sector: Probing the Extended Parameter Space","url":"/paper/2105.08744","section":"IceCube's data and analysis method","sentence":"We use the bin-averaged atmospheric neutrino fluxes $Φ^ν_μ_ik$ provided by the IceCube, based on [ref] , that have been used in the analysis of this data set and include also the corrections for the simulated detector optical efficiency, $η_ijk$, that should be multiplied by the effective areas.","intent_p":0.93,"contests_p":null},{"arxiv_id":"1108.4360","title":"Atmospheric neutrinos as a probe of eV^2-scale active-sterile oscillations","url":"/paper/1108.4360","section":"Atmospheric down-going muon neutrinos and the sterile-scale oscillation","sentence":"The atmospheric fluxes are taken from the 3-dimensional calculation in [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"1206.0328","title":"Evidence for the Appearance of Atmospheric Tau Neutrinos in Super-Kamiokande","url":"/paper/1206.0328","section":"Introduction","sentence":"Three-dimensional neutrino fluxes for and produced in atmospheric showers are taken from the flux calculation of Honda et al. [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"1811.01310","title":"Activating the 4th Neutrino of the 3+1 Scheme","url":"/paper/1811.01310","section":"The Atmospheric Neutrino Constraint from IceCube","sentence":"The atmospheric flux is provided by [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"1801.06075","title":"Detection of the Characteristic Pion-Decay Signature in the Molecular Clouds","url":"/paper/1801.06075","section":"Discussion","sentence":"The enhancement of 1.78 accounted for the nuclei heavier than He in both the ISM and the CR is also considered [ref] .","intent_p":0.89,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":2,"sentences":2,"quotes":[{"arxiv_id":"0707.1218","title":"Potentialities of atmospheric neutrinos","url":"/paper/0707.1218","section":"Direct determination of atmospheric fluxes","sentence":"In Fig. [ref] we show the results of our fit to the atmospheric neutrino flux as compared with the computations of the Honda [ref] and Bartol [ref] groups.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1510.08127","title":"Measurements of the atmospheric neutrino flux by Super-Kamiokande: energy spectra, geomagnetic effects, and solar modulation","url":"/paper/1510.08127","section":"Results and Discussion","sentence":"The prediction of the asymmetry strength is somewhat higher than in the previous SK analysis [ref] , at which time the flux simulation considered geomagnetic effects on the primary cosmic ray particles only; the additional consideration of the bending of secondary cosmic rays in the atmosphere is seen to further enhance the dipole asymmetry prediction [ref] .","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"0912.1385","title":"High energy leptons from muons in transit","url":"/paper/0912.1385","section":"Atmospheric lepton fluxes","sentence":"Atmospheric lepton fluxes come from cosmic ray interactions in the atmosphere, producing mesons which decay to leptons [ref] .","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":23},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. 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