All Tables

Table 1: Information on the photometric observations.
Table 2: Results of the photometric calibration of BVR data.
Table 3: Fits to the Luminosity Functions. Errors on the M^* and $\alpha$ parameters can be obtained by the confidence contours shown in Fig. 3.
Table 4: Best fit value of the LFs measured in three regions around the center of the cluster.
Table 5: Compilation of dip positions in the restframe R band in cluster LFs from literature. Data were transformed to R-band absolute magnitudes by using k- and evolutionary correction, and average colours for early-type galaxies of Poggianti (1997).