{"arxiv_id":"1103.4257","incoming":{"papers":1,"sentences":1,"groups":[{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2405.03308","title":"Statistical Equivalence of Metrics for Meteor Dynamical Association","url":"/paper/2405.03308","section":"Introduction","sentence":"According to the theory of formation and evolution of small bodies of the Solar System [ref] , meteoroid streams are formed mainly as a result of the activity of comets or the ejection of meteoroids from cometary nuclei with various initial velocities [ref] .","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":0},"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/1103.4257"}}