{"arxiv_id":"2210.09156","incoming":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"outgoing":{"papers":4,"sentences":7,"groups":[{"kind":"background","label":"Cites as background","papers":3,"sentences":3,"quotes":[{"arxiv_id":"2206.06161","title":"Strong C IV emission from star-forming galaxies: a case for high Lyman continuum photon escape","url":"/paper/2206.06161","section":"Introduction","sentence":"These include high O$_32$ ratios [ref] , Ly$α$ peak separations [ref] , SII deficits [ref] , MgII doublet flux ratios [ref] , strong C iv emission [ref] , the combination of H$β$ and UV slope [ref] , etc.","intent_p":0.86,"contests_p":null},{"arxiv_id":"2201.02636","title":"A survey of high-$z$ galaxies: SERRA simulations","url":"/paper/2201.02636","section":"Implications for [CII] 158$μ$m Emission","sentence":"These include the impact of the CMB and low metallicity [ref] , radiation field intensity [ref] , and bursty star formation [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"2201.11716","title":"The Low-Redshift Lyman Continuum Survey I: New, Diverse Local Lyman-Continuum Emitters","url":"/paper/2201.11716","section":"Introduction","sentence":"Rather observational studies of $f_esc$ often target lower redshift analogues of high-redshift galaxies at $z∼0$ [ref] , $z∼3$ [ref] , and more recently at $z∼1.5$ [ref] .","intent_p":0.86,"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/2210.09156"}}