  We compute the luminosity function of galaxies in groups. The data consists
in two samples of groups of galaxies selected in distance and redshift space
comprising a total number of 66 groups. The assignment of galaxies to the
groups were derived from the Edinburgh-Durham Southern Galaxy Catalog,
considering a limiting apparent magnitude $m_{lim}=19.4$.
  We find a flat faint end of the mean galaxy luminosity function in groups in
contrast to the mean galaxy LF in clusters where a large relative number of
faint galaxies is present. We find that a Schechter function with parameters
$M^{*}\simeq -19.6\pm 0.2,$ $\alpha \simeq -1.0\pm $ 0.2 provides a
satisfactory fit to the galaxy LF of our total sample of groups in the range of
absolute magnitudes $-22<M<-16$.
