{"arxiv_id":"astro-ph/0411363","incoming":{"papers":3,"sentences":3,"groups":[{"kind":"background","label":"Cites it as background","papers":3,"sentences":3,"quotes":[{"arxiv_id":"1202.4296","title":"Time dependent embedding of spherically symmetric Rindler-like spacetime","url":"/paper/1202.4296","section":"Introduction","sentence":"The solution depends upon the model of the universe [ref] .","intent_p":0.93,"contests_p":null},{"arxiv_id":"2303.17516","title":"Reference frames in General Relativity and the galactic rotation curves","url":"/paper/2303.17516","section":"PN approximation: the IAU reference systems","sentence":"Modifications of the IAU system for accommodating cosmological effects have been proposed in [ref] , by taking the cosmological expansion as a (tidal) perturbation around the PN metric [ref] [ref] , or by considering perturbations around the flat ($k=1$) subcase of the FLRW solution [ref] .","intent_p":0.84,"contests_p":null},{"arxiv_id":"1202.2285","title":"Conformal time dependent Painleve-Gullstrand spacetime","url":"/paper/1202.2285","section":"Introduction","sentence":"The apparently simple question whether the cosmological expansion takes place even locally (at the level of an atom or of the Solar System) is a very complicate one and is still an unsolved problem [ref] .","intent_p":0.9,"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/astro-ph/0411363"}}