All Tables

Table 1: Number of galaxies in the FDF for the redshift intervals used for computing the LFs. Note that we derived the LF in all redshift bins, but excluded the lowest (z < 0.45) and highest redshift bins (z > 3.81) from our analysis of the LF evolution, since the lowest redshift bin corresponds to too small a volume, while the z>3.81 bin suffers from extrapolation errors.
Table 2: Slope of the LF for all wavelengths and all redshifts as derived from a 3-parameter Schechter fit.
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.
Table 4: Luminosity densities in the UV and i' bands for the four SED types. See also Fig. 5.
Table 5: Slope of the UV (2800 Å) and i' band LF for the different SED types from a 3-parameter Schechter fit. The Schechter functions are shown in Fig. 4.
Table 6: Schechter function fit in the r'-band.
Table 7: Schechter function fit in the i'-band.
Table 8: Schechter function fit in the z'-band.
Table 9: Evolution parameters according to Eq. (1).