{"arxiv_id":"1104.5056","incoming":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"outgoing":{"papers":2,"sentences":7,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1104.5055","title":"Heavy Element Dispersion in the Metal-Poor Globular Cluster M92","url":"/paper/1104.5055","section":"Literature Data","sentence":"lccccc Correlations among Abundance Ratios 0pt Cluster (References) 5cRatio Pair 2-6 [La/Fe] $+$ [Eu/Fe] [La/Fe] $+$ [Na/Fe] [Eu/Fe] $+$ [Na/Fe] M3 [ref] (0.64, 20, 0.00024) ($-$0.20, 20, 0.39) (0.12, 22, 0.60) M3 [ref] (0.35, 7, 0.45) ($-$0.21, 7, 0.65) ($-$0.24, 8, 0.57) M5 [ref] (0.43, 25, 0.034) ($-$0.25, 25, 0.22) ($-$0.16, 25, 0.45) M5 [ref] (0.80, 17, 0.00010) (0.10, 17, 0.70) (0.16, 17, 0.55) M12 [ref] (-0.31, 21, 0.17) ($-$0.37, 11, 0.26) (0.41, 11, 0.21) M13 [ref] (0.72, 18, 0.00066) ($-$0.51, 18, 0.029) ($-$0.40, 18, 0.099) M13 [ref] (0.07, 11, 0.83) ($-$0.23, 12, 0.47) (0.43, 12, 0.16) M15 [ref] (0.97, 6, 0.0011) M15 [ref] (0.89, 9, 0.0012) (0.02, 9, 0.95) ($-$0.12, 9, 0.77) M22 [ref] a ($-$0.07, 21, 0.75) ($-$0.13, 21, 0.56) (0.21, 21, 0.36) M80 [ref] (0.37, 8, 0.37) (0.23, 10, 0.52)b (0.66, 8, 0.075)b M92 [ref] (0.49, 16, 0.052) ($-$0.02, 13, 0.95) ($-$0.24, 12, 0.45) NGC 1","intent_p":0.98,"contests_p":null},{"arxiv_id":"1105.1523","title":"The two metallicity groups of the globular cluster M22: a chemical perspective","url":"/paper/1105.1523","section":"Literature Data","sentence":"lccccc Correlations among Abundance Ratios 0pt Cluster (References) 5cRatio Pair 2-6 [La/Fe] $+$ [Eu/Fe] [La/Fe] $+$ [Na/Fe] [Eu/Fe] $+$ [Na/Fe] M3 [ref] (0.64, 20, 0.00024) ($-$0.20, 20, 0.39) (0.12, 22, 0.60) M3 [ref] (0.35, 7, 0.45) ($-$0.21, 7, 0.65) ($-$0.24, 8, 0.57) M5 [ref] (0.43, 25, 0.034) ($-$0.25, 25, 0.22) ($-$0.16, 25, 0.45) M5 [ref] (0.80, 17, 0.00010) (0.10, 17, 0.70) (0.16, 17, 0.55) M12 [ref] (-0.31, 21, 0.17) ($-$0.37, 11, 0.26) (0.41, 11, 0.21) M13 [ref] (0.72, 18, 0.00066) ($-$0.51, 18, 0.029) ($-$0.40, 18, 0.099) M13 [ref] (0.07, 11, 0.83) ($-$0.23, 12, 0.47) (0.43, 12, 0.16) M15 [ref] (0.97, 6, 0.0011) M15 [ref] (0.89, 9, 0.0012) (0.02, 9, 0.95) ($-$0.12, 9, 0.77) M22 [ref] a ($-$0.07, 21, 0.75) ($-$0.13, 21, 0.56) (0.21, 21, 0.36) M80 [ref] (0.37, 8, 0.37) (0.23, 10, 0.52)b (0.66, 8, 0.075)b M92 [ref] (0.49, 16, 0.052) ($-$0.02, 13, 0.95) ($-$0.24, 12, 0.45) NGC 1","intent_p":0.98,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1104.5055","title":"Heavy Element Dispersion in the Metal-Poor Globular Cluster M92","url":"/paper/1104.5055","section":"Introduction","sentence":"M15 and M92 show an unmistakable star-to-star dispersion of material relative to Fe (e.g., [ref] ), which is uncorrelated with the light element dispersion (see also [ref] ).","intent_p":0.96,"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/1104.5056"}}