Matches in SemOpenAlex for { <https://semopenalex.org/work/W2494814912> ?p ?o ?g. }
- W2494814912 endingPage "2848" @default.
- W2494814912 startingPage "2833" @default.
- W2494814912 abstract "We use the halo occupation distribution (HOD) framework to characterise the predictions from two independent galaxy formation models for the galactic content of dark matter haloes and its evolution with redshift. Our galaxy samples correspond to a range of fixed number densities defined by stellar mass and span $0 le z le 3$. We find remarkable similarities between the model predictions. Differences arise at low galaxy number densities which are sensitive to the treatment of heating of the hot halo by active galactic nuclei. The evolution of the form of the HOD can be described in a relatively simple way, and we model each HOD parameter using its value at $z=0$ and an additional evolutionary parameter. In particular, we find that the ratio between the characteristic halo masses for hosting central and satellite galaxies can serve as a sensitive diagnostic for galaxy evolution models. Our results can be used to test and develop empirical studies of galaxy evolution and can facilitate the construction of mock galaxy catalogues for future surveys." @default.
- W2494814912 created "2016-08-23" @default.
- W2494814912 creator A5012749486 @default.
- W2494814912 creator A5040727635 @default.
- W2494814912 creator A5041585242 @default.
- W2494814912 creator A5045186703 @default.
- W2494814912 creator A5052786955 @default.
- W2494814912 date "2016-11-03" @default.
- W2494814912 modified "2023-09-28" @default.
- W2494814912 title "The evolution of the galaxy content of dark matter haloes" @default.
- W2494814912 cites W1487343513 @default.
- W2494814912 cites W1513075382 @default.
- W2494814912 cites W1569544657 @default.
- W2494814912 cites W1607306679 @default.
- W2494814912 cites W1724036414 @default.
- W2494814912 cites W1802083559 @default.
- W2494814912 cites W1897231400 @default.
- W2494814912 cites W1907949623 @default.
- W2494814912 cites W1913372524 @default.
- W2494814912 cites W1919617765 @default.
- W2494814912 cites W1929623410 @default.
- W2494814912 cites W1935774584 @default.
- W2494814912 cites W1938555805 @default.
- W2494814912 cites W1965779302 @default.
- W2494814912 cites W1969388479 @default.
- W2494814912 cites W1976620664 @default.
- W2494814912 cites W1977102999 @default.
- W2494814912 cites W1978163182 @default.
- W2494814912 cites W1978425005 @default.
- W2494814912 cites W1980269917 @default.
- W2494814912 cites W1982230955 @default.
- W2494814912 cites W1982576080 @default.
- W2494814912 cites W1984336612 @default.
- W2494814912 cites W1991435657 @default.
- W2494814912 cites W1993501365 @default.
- W2494814912 cites W1993805366 @default.
- W2494814912 cites W1994813563 @default.
- W2494814912 cites W2000310419 @default.
- W2494814912 cites W2005730006 @default.
- W2494814912 cites W2008237982 @default.
- W2494814912 cites W2018719255 @default.
- W2494814912 cites W2022531822 @default.
- W2494814912 cites W2030612271 @default.
- W2494814912 cites W2032469582 @default.
- W2494814912 cites W2035000458 @default.
- W2494814912 cites W2040393541 @default.
- W2494814912 cites W2043425843 @default.
- W2494814912 cites W2044331057 @default.
- W2494814912 cites W2055156211 @default.
- W2494814912 cites W2058960172 @default.
- W2494814912 cites W2063867713 @default.
- W2494814912 cites W2064377583 @default.
- W2494814912 cites W2077054687 @default.
- W2494814912 cites W2079307141 @default.
- W2494814912 cites W2090459210 @default.
- W2494814912 cites W2096981162 @default.
- W2494814912 cites W2099155119 @default.
- W2494814912 cites W2102600871 @default.
- W2494814912 cites W2105453249 @default.
- W2494814912 cites W2109146631 @default.
- W2494814912 cites W2117940530 @default.
- W2494814912 cites W2125546908 @default.
- W2494814912 cites W2126510815 @default.
- W2494814912 cites W2129489826 @default.
- W2494814912 cites W2132646102 @default.
- W2494814912 cites W2139286411 @default.
- W2494814912 cites W2141138389 @default.
- W2494814912 cites W2141709306 @default.
- W2494814912 cites W2142432812 @default.
- W2494814912 cites W2145851029 @default.
- W2494814912 cites W2153156829 @default.
- W2494814912 cites W2157544440 @default.
- W2494814912 cites W2160197565 @default.
- W2494814912 cites W2162446715 @default.
- W2494814912 cites W2165233299 @default.
- W2494814912 cites W2166493535 @default.
- W2494814912 cites W2167009888 @default.
- W2494814912 cites W2167156940 @default.
- W2494814912 cites W2167388685 @default.
- W2494814912 cites W2169910932 @default.
- W2494814912 cites W2193432253 @default.
- W2494814912 cites W2197026494 @default.
- W2494814912 cites W2280547448 @default.
- W2494814912 cites W2953228579 @default.
- W2494814912 cites W3098140412 @default.
- W2494814912 cites W3098804119 @default.
- W2494814912 cites W3099471130 @default.
- W2494814912 cites W3100669571 @default.
- W2494814912 cites W3100695352 @default.
- W2494814912 cites W3101247804 @default.
- W2494814912 cites W3101621635 @default.
- W2494814912 cites W3101650711 @default.
- W2494814912 cites W3103018756 @default.
- W2494814912 cites W3103101999 @default.
- W2494814912 cites W3103374343 @default.
- W2494814912 cites W3104080146 @default.
- W2494814912 cites W3104554423 @default.
- W2494814912 cites W3104639138 @default.