Fig. 16.
Median of n as a function of sSFR for the field galaxies (blue) and the central (solid) and satellite (dashed) HB11 (orange), HB12 (green), and HB13 (red) groups. The satellite galaxies closely follow the field galaxies while the central galaxies have higher n at low sSFR. Error bars for satellite galaxies are omitted for clarity of the plot but are comparable to the errors of the central galaxies.
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