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The influence of halo assembly on galaxies and galaxy groups

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Academic year: 2020

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Figure 1. Dependence of halo age on mass-to-light ratio (top-left panel), fraction of red galaxies (top-right panel), on group inner density using the five brightest galaxies in the group (bottom-left panel) and isolation in terms of the group virial radiu
Figure 2. Dependence of group mass on concentration (right-hand panel) and group isolation (left-hand panel) for groups in the SDSS and mock catalogues.
Figure 4. Dependence of mass-to-light ratios on group concentration (left-hand panel) and isolation (right-hand panel) for mock and SDSS (filled and open symbols, respectively) groups, in two narrow ranges of halo mass (high masses are shown in upward poin
Figure 5. Dependence of the number of galaxy members on group concentration (left-hand panel) and isolation (right-hand panel) for mock and SDSS-DR6 groups (filled and open symbols, respectively), in two narrow ranges of halo mass (high masses are shown in
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