{"arxiv_id":"1204.3931","incoming":{"papers":1,"sentences":2,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1403.4754","title":"The Evolution of Compact Binary Star Systems","url":"/paper/1403.4754","section":"Formation of stars and end products of their evolution","sentence":"Modern studies suggest that for solar metallicity models it does not exceed $1.2$ [ref] .","intent_p":0.93,"contests_p":null}]}],"unlabelled_sentences":1},"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/1204.3931"}}