We present the GALEX NUV ( 2310 \AA ) and FUV ( 1530 \AA ) galaxy luminosity functions of the nearby cluster of galaxies A1367 in the magnitude range -20.3 \leq M _ { AB } \leq - 13.3 .
The luminosity functions are consistent with previous ( \sim 2 mag shallower ) estimates based on the FOCA and FAUST experiments , but display a steeper faint-end slope than the GALEX luminosity function for local field galaxies .
Using spectro-photometric optical data we select out star-forming systems from quiescent galaxies and study their separate contributions to the cluster luminosity function .
We find that the UV luminosity function of cluster star-forming galaxies is consistent with the field .
The difference between the cluster and field LF is entirely due to the contribution at low luminosities ( M _ { AB } > -16 mag ) of non star-forming , early-type galaxies that are significantly over dense in clusters .