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• W3084652075 abstract "How do galaxy properties (such as stellar mass, luminosity, star formation rate, and morphology) and their evolution depend on the mass of their host dark matter halo? Using the Galaxy and Mass Assembly (GAMA) group catalogue, we address this question by exploring the dependence on host halo mass of the luminosity function (LF) and stellar mass function (SMF) for grouped galaxies subdivided by colour, morphology and central/satellite. We find that spheroidal galaxies in particular dominate the bright and massive ends of the LF and SMF, respectively. More massive haloes host more massive and more luminous central galaxies. The satellite LF and SMF respectively show a systematic brightening of characteristic magnitude, and increase in characteristic mass, with increasing halo mass. In contrast to some previous results, the faint-end and low-mass slopes show little systematic dependence on halo mass. Semi-analytic models and simulations show similar or enhanced dependence of central mass and luminosity on halo mass. Faint and low-mass simulated satellite galaxies are remarkably independent of halo mass, but the most massive satellites are more common in more massive groups. In the first investigation of low-redshift LF and SMF evolution in group environments, we find that the red/blue ratio of galaxies in groups has increased since redshift $z approx 0.3$ relative to the field population. This observation strongly suggests that quenching of star formation in galaxies as they are accreted into galaxy groups is a significant and ongoing process." @default.
• W3084652075 created "2020-09-21" @default.
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• W3084652075 date "2020-09-21" @default.
• W3084652075 modified "2023-10-13" @default.
• W3084652075 title "Galaxy and mass assembly: luminosity and stellar mass functions in GAMA groups" @default.
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• W3084652075 cites W1847269195 @default.
• W3084652075 cites W1867260751 @default.
• W3084652075 cites W1879552933 @default.
• W3084652075 cites W1879615959 @default.
• W3084652075 cites W1882683373 @default.
• W3084652075 cites W1911962099 @default.
• W3084652075 cites W1916636306 @default.
• W3084652075 cites W1922047266 @default.
• W3084652075 cites W1929623410 @default.
• W3084652075 cites W1966926090 @default.
• W3084652075 cites W1967037608 @default.
• W3084652075 cites W1973368884 @default.
• W3084652075 cites W1976637727 @default.
• W3084652075 cites W1978163182 @default.
• W3084652075 cites W1982555406 @default.
• W3084652075 cites W1988235022 @default.
• W3084652075 cites W1999367759 @default.
• W3084652075 cites W2000560393 @default.
• W3084652075 cites W2002399119 @default.
• W3084652075 cites W2006284873 @default.
• W3084652075 cites W2015637674 @default.
• W3084652075 cites W2018828554 @default.
• W3084652075 cites W2023873184 @default.
• W3084652075 cites W2024297548 @default.
• W3084652075 cites W2024370579 @default.
• W3084652075 cites W2028715663 @default.
• W3084652075 cites W2040520625 @default.
• W3084652075 cites W2042179541 @default.
• W3084652075 cites W2042483343 @default.
• W3084652075 cites W2046149262 @default.
• W3084652075 cites W2059407430 @default.
• W3084652075 cites W2066499352 @default.
• W3084652075 cites W2070081597 @default.
• W3084652075 cites W2074106980 @default.
• W3084652075 cites W2085094825 @default.
• W3084652075 cites W2090459210 @default.
• W3084652075 cites W2091390718 @default.
• W3084652075 cites W2091677451 @default.
• W3084652075 cites W2092571324 @default.
• W3084652075 cites W2094139033 @default.
• W3084652075 cites W2103612329 @default.
• W3084652075 cites W2111817932 @default.
• W3084652075 cites W2114553120 @default.
• W3084652075 cites W2115527611 @default.
• W3084652075 cites W2119131940 @default.
• W3084652075 cites W2126510815 @default.
• W3084652075 cites W2138616264 @default.
• W3084652075 cites W2140681319 @default.
• W3084652075 cites W2141709306 @default.
• W3084652075 cites W2142238829 @default.
• W3084652075 cites W2148719886 @default.
• W3084652075 cites W2151008701 @default.
• W3084652075 cites W2157917411 @default.
• W3084652075 cites W2159710473 @default.
• W3084652075 cites W2166493535 @default.
• W3084652075 cites W2170649168 @default.
• W3084652075 cites W2170689655 @default.
• W3084652075 cites W2185926565 @default.
• W3084652075 cites W2194108049 @default.
• W3084652075 cites W2197026494 @default.
• W3084652075 cites W2337947861 @default.
• W3084652075 cites W2529434142 @default.
• W3084652075 cites W2613638711 @default.
• W3084652075 cites W2618531798 @default.
• W3084652075 cites W2734538553 @default.
• W3084652075 cites W2735189638 @default.
• W3084652075 cites W2735395126 @default.
• W3084652075 cites W2735531560 @default.
• W3084652075 cites W2735710795 @default.
• W3084652075 cites W2750749672 @default.
• W3084652075 cites W2792981659 @default.
• W3084652075 cites W2807865283 @default.
• W3084652075 cites W2883820818 @default.

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