{"arxiv_id":"gr-qc/0001077","incoming":{"papers":3,"sentences":4,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2306.17265","title":"Generic initial data for binary boson stars","url":"/paper/2306.17265","section":"Modified superposition","sentence":"In the case of binary black hole or neutron star initial data, it is common practice to remove the metric variables of one star at the location of the other (analogous to approaches introduced in Refs. [ref] ), achieved by non-trivial attenuation functions $f_(A)$.","intent_p":0.86,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":1,"sentences":2,"quotes":[{"arxiv_id":"0812.3132","title":"Reducing spurious gravitational radiation in binary-black-hole simulations by using conformally curved initial data","url":"/paper/0812.3132","section":"Introduction","sentence":"Note that the superposed metrics in this paper and in Ref. [ref] are similar to the superposed-Kerr-Schild conformal metrics used in Refs. [ref] ; however, the conformal metrics used here and in Ref. [ref] are flat everywhere except near each black hole.","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/gr-qc/0001077"}}