{"arxiv_id":"hep-ph/0305208","incoming":{"papers":6,"sentences":7,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1004.1008","title":"Lifetime Constraints for Late Dark Matter Decay","url":"/paper/1004.1008","section":"Decay into neutrinos.","sentence":"We utilize the results of the FLUKA [ref] calculation of the atmospheric $_+ _$ background, over the energy range 50 MeV to 10 TeV.","intent_p":0.87,"contests_p":null},{"arxiv_id":"1111.6041","title":"Neutrino Signals from Gravitino Dark Matter with Broken R-Parity","url":"/paper/1111.6041","section":"Atmospheric Neutrinos","sentence":"For the energy range 25–10000GeV only the muon neutrino flux is available [ref] .","intent_p":1.0,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1502.03916","title":"Atmospheric neutrino flux calculation using the NRLMSISE00 atmospheric model","url":"/paper/1502.03916","section":"introduction","sentence":"The US-standard '76 atmospheric model had been used generally in the study of cosmic rays in the atmosphere for a long time [ref] .","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":4},"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. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":null,"_links":{"html":"https://pith.science/paper/hep-ph/0305208"}}