All Tables

Table 1: Photometric parameters of optical data.
Table 2: Fits to the LFs for cluster galaxies. Errors on the M^* and $\alpha$ parameters are indicated by the confidence contours shown in Figs. 5, 7 and 9.
Table 3: Fits to the red sequence galaxy LFs. Errors on the R^* and $\alpha$ parameters are indicated by the confidence contours shown in Figs. 10 and 12.