{"arxiv_id":"1402.2405","incoming":{"papers":5,"sentences":6,"groups":[{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2604.22703","title":"Reionization, UV Luminosity and 21$\\,$cm Sensitivity to Primordial Magnetic Fields: Impact of Energy Losses","url":"/paper/2604.22703","section":"Introduction","sentence":"The presence of PMFs would also have impacted galaxy and star formation processes [ref] .","intent_p":0.88,"contests_p":null},{"arxiv_id":"1708.02477","title":"On the implementation of the spherical collapse model for dark energy models","url":"/paper/1708.02477","section":"Introduction","sentence":"Finally, [ref] studied the spherical collapse model taking into consideration the effect of neutrinos and [ref] the effects of primordial magnetic fields.","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":4},"outgoing":{"papers":9,"sentences":9,"groups":[{"kind":"background","label":"Cites as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"astro-ph/0502283","title":"Magnetic field generation from cosmological perturbations","url":"/paper/astro-ph/0502283","section":"Introduction","sentence":"A variety of mechanisms for PMF generation has been proposed, such as inflation, phase transitions in the early universe and cosmological vector modes [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"astro-ph/0603631","title":"Cosmological Magnetic Field: a fossil of density perturbations in the early universe","url":"/paper/astro-ph/0603631","section":"Introduction","sentence":"A variety of mechanisms for PMF generation has been proposed, such as inflation, phase transitions in the early universe and cosmological vector modes [ref] .","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":7},"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/1402.2405"}}