Matches in SemOpenAlex for { <https://semopenalex.org/work/W2765188034> ?p ?o ?g. }
- W2765188034 endingPage "758" @default.
- W2765188034 startingPage "741" @default.
- W2765188034 abstract "SubHalo Abundance Matching (SHAM) assumes that one (sub)halo property, such as mass Mvir or peak circular velocity Vpeak, determines properties of the galaxy hosted in each (sub)halo such as its luminosity or stellar mass. This assumption implies that the dependence of Galaxy Luminosity Functions (GLFs) and the Galaxy Stellar Mass Function (GSMF) on environmental density is determined by the corresponding halo density dependence. In this paper, we test this by determining from an SDSS sample the observed dependence with environmental density of the ugriz GLFs and GSMF for all galaxies, and for central and satellite galaxies separately. We then show that the SHAM predictions are in remarkable agreement with these observations, even when the galaxy population is divided between central and satellite galaxies. However, we show that SHAM fails to reproduce the correct dependence between environmental density and g-r color for all galaxies and central galaxies, although it better reproduces the color dependence on environmental density of satellite galaxies." @default.
- W2765188034 created "2017-11-10" @default.
- W2765188034 creator A5003955384 @default.
- W2765188034 creator A5020498630 @default.
- W2765188034 creator A5040010680 @default.
- W2765188034 creator A5041746582 @default.
- W2765188034 date "2018-02-02" @default.
- W2765188034 modified "2023-10-02" @default.
- W2765188034 title "Does the galaxy–halo connection vary with environment?" @default.
- W2765188034 cites W1520258040 @default.
- W2765188034 cites W1827769868 @default.
- W2765188034 cites W1881487679 @default.
- W2765188034 cites W1882683373 @default.
- W2765188034 cites W1883767967 @default.
- W2765188034 cites W1915403329 @default.
- W2765188034 cites W1964055719 @default.
- W2765188034 cites W1965779302 @default.
- W2765188034 cites W1966876239 @default.
- W2765188034 cites W1982505278 @default.
- W2765188034 cites W1986837390 @default.
- W2765188034 cites W1988235022 @default.
- W2765188034 cites W1997812697 @default.
- W2765188034 cites W1997959519 @default.
- W2765188034 cites W2000310419 @default.
- W2765188034 cites W2005720343 @default.
- W2765188034 cites W2007978190 @default.
- W2765188034 cites W2021815414 @default.
- W2765188034 cites W2023351067 @default.
- W2765188034 cites W2028715663 @default.
- W2765188034 cites W2033070170 @default.
- W2765188034 cites W2033529120 @default.
- W2765188034 cites W2033933651 @default.
- W2765188034 cites W2035000458 @default.
- W2765188034 cites W2037342525 @default.
- W2765188034 cites W2039804150 @default.
- W2765188034 cites W2042483343 @default.
- W2765188034 cites W2048116537 @default.
- W2765188034 cites W2059407430 @default.
- W2765188034 cites W2065353414 @default.
- W2765188034 cites W2069685156 @default.
- W2765188034 cites W2073469924 @default.
- W2765188034 cites W2073501758 @default.
- W2765188034 cites W2074259895 @default.
- W2765188034 cites W2075026317 @default.
- W2765188034 cites W2077054687 @default.
- W2765188034 cites W2080348355 @default.
- W2765188034 cites W2080927107 @default.
- W2765188034 cites W2088461970 @default.
- W2765188034 cites W2114553120 @default.
- W2765188034 cites W2126510815 @default.
- W2765188034 cites W2127193056 @default.
- W2765188034 cites W2141771434 @default.
- W2765188034 cites W2147357138 @default.
- W2765188034 cites W2153094038 @default.
- W2765188034 cites W2157544440 @default.
- W2765188034 cites W2158622701 @default.
- W2765188034 cites W2159710473 @default.
- W2765188034 cites W2169910932 @default.
- W2765188034 cites W2280547448 @default.
- W2765188034 cites W2313105505 @default.
- W2765188034 cites W2518944150 @default.
- W2765188034 cites W2530063092 @default.
- W2765188034 cites W2547700289 @default.
- W2765188034 cites W2597801633 @default.
- W2765188034 cites W2613638711 @default.
- W2765188034 cites W3098575811 @default.
- W2765188034 cites W3098804119 @default.
- W2765188034 cites W3098844796 @default.
- W2765188034 cites W3099871027 @default.
- W2765188034 cites W3100024326 @default.
- W2765188034 cites W3100383694 @default.
- W2765188034 cites W3100987161 @default.
- W2765188034 cites W3101369122 @default.
- W2765188034 cites W3101475602 @default.
- W2765188034 cites W3101926670 @default.
- W2765188034 cites W3102987263 @default.
- W2765188034 cites W3104746642 @default.
- W2765188034 cites W3105014804 @default.
- W2765188034 cites W3105465984 @default.
- W2765188034 cites W3105554724 @default.
- W2765188034 cites W3105631369 @default.
- W2765188034 cites W3106072945 @default.
- W2765188034 cites W3106274511 @default.
- W2765188034 cites W3106456019 @default.
- W2765188034 cites W3121922651 @default.
- W2765188034 cites W3124530745 @default.
- W2765188034 cites W3126142052 @default.
- W2765188034 doi "https://doi.org/10.1093/mnras/sty283" @default.
- W2765188034 hasPublicationYear "2018" @default.
- W2765188034 type Work @default.
- W2765188034 sameAs 2765188034 @default.
- W2765188034 citedByCount "25" @default.
- W2765188034 countsByYear W27651880342018 @default.
- W2765188034 countsByYear W27651880342019 @default.
- W2765188034 countsByYear W27651880342020 @default.
- W2765188034 countsByYear W27651880342021 @default.
- W2765188034 countsByYear W27651880342022 @default.
- W2765188034 countsByYear W27651880342023 @default.