Table 3: In the upper part of the table, we show the slope $\alpha$ of the luminosity functions for the different wavebands as determined from an error-weighted fit to the data, under the assumption that $\alpha(z)={\rm const.}$ In the lower part of the table, we show the best values of $\alpha$ after combining the data of all bands.
Filter $\alpha(z)={\rm const.}$

r' $-1.30 \pm 0.05$

i' $-1.33 \pm 0.05$

z' $-1.35 \pm 0.05$

r' & i' & z' $-1.33 \pm 0.03$

**Table 3:** In the upper part of the table, we show the slope $\alpha$ of the luminosity functions for the different wavebands as determined from an error-weighted fit to the data, under the assumption that $\alpha(z)={\rm const.}$ In the lower part of the table, we show the best values of $\alpha$ after combining the data of all bands.
Filter	$\alpha(z)={\rm const.}$
r'	$-1.30 \pm 0.05$
i'	$-1.33 \pm 0.05$
z'	$-1.35 \pm 0.05$
r' & i' & z'	$-1.33 \pm 0.03$

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