Table 1: Galaxy distribution in the FDF for the redshift intervals used for computing the luminosity function. Note that we derive the luminosity function in all redshift bins, but exclude the lowest (z < 0.45) and highest redshift bin (z > 5.01) from our analysis of the luminosity function evolution, since the lowest redshift bin corresponds to a too small volume while the z>5.01 bin suffers from incompleteness.

Redshift	Number	Fraction
interval	of galaxies	of galaxies
0.00-0.45	808	14.54%
0.45-0.81	998	17.96%
0.81-1.11	885	15.92%
1.11-1.61	898	16.16%
1.61-2.15	504	9.07%
2.15-2.91	746	13.42%
2.91-4.01	549	9.88%
4.01-5.01	150	2.70%
>5.01	18	0.32%
Unknown	2	0.04%