Fig. 5
Comparison of the IR LFs in groups (black filled points and solid lines) at 0.1 <z< 0.4 derived in this work and the group LFs of Guo et al. (2014) (red symbols and dashed lines) converted into IR LF derived at 0.1 < 0 < 0.2 (triangles), 0.2 < 0 < 0.3 (squares), and 0.3 <z< 0.4 (stars). For clarity we show here only the best fit derived with the modified Schechter function of Saunders et al. (1990).
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