{"arxiv_id":"1104.5055","incoming":{"papers":2,"sentences":6,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1104.5056","title":"Primordial r-process Dispersion in Metal-Poor Globular Clusters","url":"/paper/1104.5056","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) ($-$0.20, 20, 0.39) (0.12, 22, 0.60) M3 [ref] (0.35, 7, 0.45) ($-$0.21, 7, 0.65) ($-$0.24, 8, 0.57) M5 [ref] (0.43, 25, 0.034) ($-$0.25, 25, 0.22) ($-$0.16, 25, 0.45) M5 [ref] (0.80, 17, 0.00010) (0.10, 17, 0.70) (0.16, 17, 0.55) M12 [ref] (-0.31, 21, 0.17) ($-$0.37, 11, 0.26) (0.41, 11, 0.21) M13 [ref] (0.72, 18, 0.00066) ($-$0.51, 18, 0.029) ($-$0.40, 18, 0.099) M13 [ref] (0.07, 11, 0.83) ($-$0.23, 12, 0.47) (0.43, 12, 0.16) M15 [ref] (0.97, 6, 0.0011) M15 [ref] (0.89, 9, 0.0012) (0.02, 9, 0.95) ($-$0.12, 9, 0.77) M22 [ref] a ($-$0.07, 21, 0.75) ($-$0.13, 21, 0.56) (0.21, 21, 0.36) M80 [ref] (0.37, 8, 0.37) (0.23, 10, 0.52)b (0.66, 8, 0.075)b M92 [ref] (0.49, 16, 0.052) ($-$0.02, 13, 0.95) ($-$0.24, 12, 0.45) NGC 1","intent_p":0.98,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1104.5056","title":"Primordial r-process Dispersion in Metal-Poor Globular Clusters","url":"/paper/1104.5056","section":"Introduction","sentence":"M15 and M92 show an unmistakable star-to-star dispersion of material relative to Fe (e.g., [ref] ), which is uncorrelated with the light element dispersion (see also [ref] ).","intent_p":0.96,"contests_p":null}]}],"unlabelled_sentences":4},"outgoing":{"papers":2,"sentences":3,"groups":[{"kind":"background","label":"Cites as background","papers":1,"sentences":2,"quotes":[{"arxiv_id":"1105.1523","title":"The two metallicity groups of the globular cluster M22: a chemical perspective","url":"/paper/1105.1523","section":"Introduction","sentence":"While the heaviest elements in most metal-poor GCs have been produced primarily by rapid ($r$) nucleosynthesis, some GCs have been enriched by a significant amount of material produced in the slow ($s$) process (M4, [ref] , [ref] ; M22, [ref] ; , [ref] , [ref] , [ref] , [ref] ; $ω$ Centauri, e.g., [ref] , [ref] ).","intent_p":0.83,"contests_p":null}]}],"unlabelled_sentences":1},"claims":[{"relation":"contradicts","label":"States a conflicting result","papers":[{"arxiv_id":"1109.2876","url":"/paper/1109.2876","title":"No Heavy Element Dispersion in the Globular Cluster M92","main_claim":"Although there have been recent claims that there is a large dispersion in the abundances of the heavy neutron capture elements in the old Galactic globular cluster M92, we show that the measured dispersion for the absolute abundances of four of the rare earth elements within a sample of 12 luminous red giants in M92 (less than or equal to 0.07 dex) does not exceed the relevant sources of uncertainty.","p":0.97}]}],"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/1104.5055"}}