{"arxiv_id":"1003.0835","incoming":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"outgoing":{"papers":7,"sentences":25,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1002.3660","title":"Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation","url":"/paper/1002.3660","section":"Connection between the observational VDF and the HMF from N-body simulations","sentence":"By relating the maximum circular velocity to the halo virial mass using the scaling given by [ref] , we find a varying fraction from $f_sub ≈0.25$ ($≈0.18$) at $10^11$ (this mass scale corresponds to the [ref] completeness limit) to $≈0.08$ ($≈0.08$) at $10^13$ for $z=0$ ($z=1$).","intent_p":0.84,"contests_p":null}]},{"kind":"comparison","label":"Compares with","papers":1,"sentences":7,"quotes":[{"arxiv_id":"1004.4626","title":"The Kinematic Connection Between Galaxies and Dark Matter Haloes","url":"/paper/1004.4626","section":"The $$-$$ relation at $z=0$","sentence":"However, our results for less massive galaxies ($10^2.3$) give systematically higher median values of $/$ compared with the [ref] results for late-type galaxies although the estimated intrinsic scatters (not shown here) overlap.","intent_p":1.0,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites as support","papers":2,"sentences":2,"quotes":[{"arxiv_id":"0903.4682","title":"Constraints on the relationship between stellar mass and halo mass at low and high redshift","url":"/paper/0903.4682","section":"Implications for the $$ paradigm and galaxy evolution","sentence":"The observation that the amount of star formation (i.e. stellar mass $$) is correlated with $$ (e.g. [ref] ) is consistent with the above picture.","intent_p":0.99,"contests_p":null},{"arxiv_id":"0909.4305","title":"How do galaxies populate Dark Matter halos?","url":"/paper/0909.4305","section":"Implications for the $$ paradigm and galaxy evolution","sentence":"The observation that the amount of star formation (i.e. stellar mass $$) is correlated with $$ (e.g. [ref] ) is consistent with the above picture.","intent_p":0.99,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":3,"sentences":3,"quotes":[{"arxiv_id":"0903.4682","title":"Constraints on the relationship between stellar mass and halo mass at low and high redshift","url":"/paper/0903.4682","section":"Introduction","sentence":"Some recent works in the literature are focused on the connection of the HMF with the broadly measured stellar mass function (SMF) of galaxies (e.g., [ref] ).","intent_p":0.98,"contests_p":null},{"arxiv_id":"0909.4305","title":"How do galaxies populate Dark Matter halos?","url":"/paper/0909.4305","section":"Introduction","sentence":"Some recent works in the literature are focused on the connection of the HMF with the broadly measured stellar mass function (SMF) of galaxies (e.g., [ref] ).","intent_p":0.98,"contests_p":null},{"arxiv_id":"1002.3660","title":"Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation","url":"/paper/1002.3660","section":"Introduction","sentence":"Accordingly, it includes the stellar mass once the galaxy is formed.] function (HMF) over cosmic time (e.g., [ref] ).","intent_p":0.84,"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/1003.0835"}}