{"arxiv_id":"1702.06546","incoming":{"papers":3,"sentences":3,"groups":[],"unlabelled_sentences":3},"outgoing":{"papers":13,"sentences":24,"groups":[{"kind":"comparison","label":"Compares with","papers":3,"sentences":5,"quotes":[{"arxiv_id":"1401.7329","title":"Stellar mass -- halo mass relation and star formation efficiency in high-mass halos","url":"/paper/1401.7329","section":"The Relation between the Stellar and Halo Mass of Central Galaxies","sentence":"Especially, the results obtained by [ref] resemble very closely the simulation result.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1605.03182","title":"Effects of Local Environment and Stellar Mass on Galaxy Quenching out to z~3","url":"/paper/1605.03182","section":"The Relation between the Environment and the Star Formation Rate","sentence":"This trend is in good agreement with observations by [ref] , who also find that at higher redshift the fraction of quiescent galaxies does not depend on the environment, while it does at low redshift.","intent_p":0.87,"contests_p":null},{"arxiv_id":"1602.01841","title":"The extended epoch of galaxy formation: age dating of ~3600 galaxies with 2<z<6.5 in the VIMOS Ultra-Deep Survey","url":"/paper/1602.01841","section":"Evolution of the SFR-$z_form$ relation","sentence":"At $z=2$ we find a median formation redshift for star-forming galaxies to be 3.36, which is in line with recent observations by [ref] , who evaluate a median formation redshift of $∼3.22$ for their galaxy sample observed at $2<z<6.5$ when using a formation redshift based on mean stellar ages similar to ours.","intent_p":0.93,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":2,"sentences":3,"quotes":[{"arxiv_id":"1401.7329","title":"Stellar mass -- halo mass relation and star formation efficiency in high-mass halos","url":"/paper/1401.7329","section":"Introduction","sentence":"Indirect measurement methods are needed to infer the halo mass from observable quantities, for example from hot X-ray halo gas [ref] , weak galaxy-galaxy lensing [ref] , satellite velocities [ref] or the number of satellites [ref] , although discrepancies exist between the results of the different methods [ref] .","intent_p":0.89,"contests_p":null},{"arxiv_id":"1607.04678","title":"The Correlation Between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe","url":"/paper/1607.04678","section":"The Relation between the Stellar and Halo Mass of Central Galaxies","sentence":"Over the past years several studies investigated the stellar-to-halo-mass relation [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":16},"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/1702.06546"}}