{"arxiv_id":"1011.1000","incoming":{"papers":2,"sentences":2,"groups":[],"unlabelled_sentences":2},"outgoing":{"papers":29,"sentences":47,"groups":[{"kind":"comparison","label":"Compares with","papers":2,"sentences":4,"quotes":[{"arxiv_id":"1007.0742","title":"Multiscale Phenomenology of the Cosmic Web","url":"/paper/1007.0742","section":"Statistics of filaments around clusters","sentence":"We find more massive halos have more filaments ending upon them, shown in Fig. [ref], bottom, just as found by [ref] with their different finders.","intent_p":0.92,"contests_p":null},{"arxiv_id":"1009.4014","title":"The persistent cosmic web and its filamentary structure II: Illustrations","url":"/paper/1009.4014","section":"Filament finder","sentence":"The work most similar to ours in focus, studying clusters as filament endpoints, is in [ref] , some related results are also found and compared in [ref] (see also [ref] , who found a cluster as an intersection of filaments in observational data).","intent_p":0.84,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":26,"sentences":31,"quotes":[{"arxiv_id":"1007.0742","title":"Multiscale Phenomenology of the Cosmic Web","url":"/paper/1007.0742","section":"Introduction","sentence":"The environments of clusters have been studied within several contexts and using several methods, e.g. galaxy and dark matter density around clusters [ref] , filamentary growth (e.g. [ref] ) around clusters, filamentary counts [ref] , in particular the geometry and properties of superclusters, e.g., [ref] , and the cluster alignment studies such as mentioned above.","intent_p":0.98,"contests_p":null},{"arxiv_id":"astro-ph/0607539","title":"Clusters and the Cosmic Web","url":"/paper/astro-ph/0607539","section":"Introduction","sentence":"The environments of clusters have been studied within several contexts and using several methods, e.g. galaxy and dark matter density around clusters [ref] , filamentary growth (e.g. [ref] ) around clusters, filamentary counts [ref] , in particular the geometry and properties of superclusters, e.g., [ref] , and the cluster alignment studies such as mentioned above.","intent_p":0.98,"contests_p":null},{"arxiv_id":"1010.0981","title":"Morphological Properties of Superclusters of Galaxies","url":"/paper/1010.0981","section":"Introduction","sentence":"The environments of clusters have been studied within several contexts and using several methods, e.g. galaxy and dark matter density around clusters [ref] , filamentary growth (e.g. [ref] ) around clusters, filamentary counts [ref] , in particular the geometry and properties of superclusters, e.g., [ref] , and the cluster alignment studies such as mentioned above.","intent_p":0.98,"contests_p":null},{"arxiv_id":"1006.4178","title":"Geometry of the Cosmic Web: Minkowski Functionals from the Delaunay Tessellation","url":"/paper/1006.4178","section":"Introduction","sentence":"The environments of clusters have been studied within several contexts and using several methods, e.g. galaxy and dark matter density around clusters [ref] , filamentary growth (e.g. [ref] ) around clusters, filamentary counts [ref] , in particular the geometry and properties of superclusters, e.g., [ref] , and the cluster alignment studies such as mentioned above.","intent_p":0.98,"contests_p":null},{"arxiv_id":"1002.3465","title":"The evolution of the density of galaxy clusters and groups: denser environments at higher redshifts","url":"/paper/1002.3465","section":"Introduction","sentence":"The environments of clusters have been studied within several contexts and using several methods, e.g. galaxy and dark matter density around clusters [ref] , filamentary growth (e.g. [ref] ) around clusters, filamentary counts [ref] , in particular the geometry and properties of superclusters, e.g., [ref] , and the cluster alignment studies such as mentioned above.","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":12},"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/1011.1000"}}