\begin{table}%T3 %\centering \par \caption{Luminosity function parameters and estimated absolute $K$~band luminosities and mass-to-light ratios. Column 2: indicative radius within which the LF and the {\it M/L}~ratio are measured; Col.~3: original passband in which the LF is measured; Col.~4: LF characteristic magnitude~$M^{*}$ as measured in the original passband, Col.~5: $M^{*}$ k-corrected to the restframe $K_{\rm s}$ band ({\it F160W} was previously corrected to $K_{\rm s}$ band by a factor $-0.5$); Col.~6: LF faint end slope $\alpha$ (note that for Cl0910 $\alpha$ is unconstrained, and the error on $M^{*}$ for this cluster is estimated assuming that $-1.4< \alpha <-0.4 $); Col.~7: the total restframe $K_{\rm s}$ luminosity within the effective area listed in Col.~6 of Table~\ref{tab:data}; Col.~8: the restframe $K_{\rm s}$ band mass-to-light ratio (the errors come from the errors on the projected mass and on the total luminosity). Note that for Cl1252 we report the total luminosity and the {\it M/L}~ratio derived from both the LFs from this work and from T04 (first and second value respectively). \label{tab:LFs} } \begin{tabular}{@{}l l l l l l l l@{}} \hline\hline Cluster&$r$&Passband&$M^{*}_{\rm obs}$&$K^{*}_{\rm rest}$&$\alpha$&$L_{K_{\rm s},