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Table 6:

Dwarf-to-giant (D/G) ratios obtained from the OLFs.
Group D/G0.5 D/G0.5,17 D/G $_{\rm WFI}$ D/G $_{\rm WFI,17}$
RR 143 1.3 $\pm$ 0.7 0.0 $\pm$ 0 1.9 $\pm$ 1.2 0.0 $\pm$ 0
RR 210 4.2 $\pm$ 1.4 1.8 $\pm$ 0.7 3.9 $\pm$ 2.1 2.0 $\pm$ 1.2
RR 216 3.0 $\pm$ 1.0 1.0 $\pm$ 0.4 8.0 $\pm$ 3.8 2.5 $\pm$ 1.4
RR 242 3.4 $\pm$ 1.1 0.9 $\pm$ 0.4 4.3 $\pm$ 1.6 0.9 $\pm$ 0.5
Combined X-ray bright 2.2 $\pm$ 0.6 0.4 $\pm$ 0.2 3.0 $\pm$ 0.9 0.4 $\pm$ 0.2
Combined X-ray faint 3.5 $\pm$ 0.8 1.3 $\pm$ 0.4 5.8 $\pm$ 2.0 2.2 $\pm$ 0.9
Column 2: D/G0.5: dwarf-to-giant ratio for galaxies within 0.5  h100-1 Mpc; Col. 3: D/G0.5,17: dwarf-to-giant ratio for galaxies within 0.5  h100-1 Mpc using only dwarfs brighter than $M_R = -17 +5~ \log h_{100}$; Col. 4: D/G $_{\rm WFI}$: dwarf-to-giant ratio for galaxies within the WFI field of view; Col. 5: D/G $_{\rm WFI,17}$: dwarf-to-giant ratio for galaxies within the WFI field of view using only dwarfs brighter than $M_R = -17 +5~ \log h_{100}$.

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