Table 3: The radio luminosity function $\rho $, in units of log(Mpc-3) per $\Delta z = 0.5$ per $\Delta ($logP) = 0.4, as derived from Sample 2, Table 2. N is the number observed per bin and $\overline {z}$ the mean redshift of the sources in the bin.

Power

0<z<0.5 0.5<z<1.0 1.0<z<2.0 2.0<z<3.0 3.0<z<5.0

log(P/ WHz-1 sr-1)

log$\rho $ N $\bar{z}$ log$\rho $ N $\bar{z}$ log$\rho $ N $\bar{z}$ log$\rho $ N $\bar{z}$ log$\rho $ N $\bar{z}$

24.8

-9.02 4 0.33 -10.22 1 0.58 - 0 - - 0 - - 0 -
25.2 -8.60 15 0.36 -9.13 6 0.62 - 0 - - 0 - - 0 -
25.6 -9.54 2 0.32 -8.91 29 0.73 -10.40 5 1.11 -11.43 1 2.12 - 0 -
26.0 -10.27 1 0.36 -9.26 19 0.77 -9.57 45 1.32 - 0 - - 0 -
26.4 -11.11 1 0.16 -9.85 15 0.78 -9.33 91 1.47 -10.34 19 2.24 -12.13 1 3.45
26.8 - 0 - -10.35 5 0.77 -10.05 29 1.69 -10.05 34 2.48 -11.02 12 3.47
27.2 - 0 - - 0 - -11.00 6 1.50 -10.98 8 2.33 -11.82 2 3.45
27.6 - 0 - - 0 - - 0 - -12.19 1 2.56 -12.32 1 3.57


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