{"arxiv_id":"2009.08611","incoming":{"papers":2,"sentences":2,"groups":[{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2010.05824","title":"Dynamical evolution of Population III stellar systems and the resulting binary statistics","url":"/paper/2010.05824","section":"Introduction","sentence":"Therefore, in the past decades, astronomers developed the machinery of binary population synthesis (BPS; see [ref] for a review), which is applied to numerous topics, such as carbon-enhanced-metal-poor (CEMP) stars (e.g. [ref] ), type Ia supernovae (SNe; e.g. [ref] ), X-ray binaries (XRBs; e.g. [ref] ), synthetic spectra of stellar populations in galaxies (e.g. [ref] ), reionization (e.g. [ref] ), and mergers of compact objects (e.g. [ref] ).","intent_p":0.92,"contests_p":null}]}],"unlabelled_sentences":1},"outgoing":{"papers":4,"sentences":4,"groups":[],"unlabelled_sentences":4},"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/2009.08611"}}