{"arxiv_id":"2104.08306","incoming":{"papers":1,"sentences":1,"groups":[],"unlabelled_sentences":1},"outgoing":{"papers":6,"sentences":7,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2012.02169","title":"A purely acceleration-based measurement of the fundamental Galactic parameters","url":"/paper/2012.02169","section":"Data","sentence":"We adopt the values from [ref] for the solar Galactocentric distance $R_⊙=8.22$, the local circular velocity $v_c = 243.0$, and the solar motion with respect to the local standard of rest $(U_⊙, V_⊙, W_⊙) = (11.10,7.20,7.25)$.","intent_p":1.0,"contests_p":null},{"arxiv_id":"2011.02505","title":"The GALAH+ Survey: Third Data Release","url":"/paper/2011.02505","section":"Data","sentence":"This Letter is based on a combination of data from the Exoplanet Archive with APOGEE DR16, GEDR3, GALAH DR3, and LAMOST DR5 ( [ref] see Appendix [ref] for details about the sample selection criteria).","intent_p":0.97,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2006.01783","title":null,"url":"/paper/2006.01783","section":"Accreted or Heated?","sentence":"The accretion event of the massive dwarf galaxy GE ( [ref] ) occurred approximately $∼$10 Gyr ago ( [ref] ) and is thought to be responsible for the formation of the thick disk either by dynamical heating ( [ref] ) or by an induced star-formation burst ( [ref] ).","intent_p":0.91,"contests_p":null}]}],"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/2104.08306"}}