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Properties of galaxy groups in the Sloan Digital Sky Survey — I. The dependence of colour, star formation and morphology on halo mass

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Academic year: 2021

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Figure 1. The upper left-hand panel shows the CM relation for the galaxies in our sample
Figure 2. Histograms of the distribution of galaxies as function of absolute r-band magnitude (upper left-hand panel), g − r colour (upper right-hand panel), SSFR (lower left-hand panel) and concentration (lower right-hand panel)
Figure 3. The fraction of late-types (open circles with blue lines), early-types (crosses with red lines) and intermediate-types (open triangles with green lines) as function of absolute magnitude (in r band, k-corrected to z = 0.1)
Figure 4. The fractions of late-types (left-hand panels), early-types (middle panels) and intermediate-types (right-hand panels) as function of their absolute magnitude
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