Table 3.
Local 150 MHz luminosity functions of AGN and SF galaxies separately.
| Radio AGN |
Star-forming galaxies |
|||
|---|---|---|---|---|
| log10L150 MHz | N | log10ρ | N | log10ρ |
| (W Hz−1) | (log10L)−1 Mpc−3 | (log10L)−1 Mpc−3 | ||
| 21.10–21.40 | 12 |
 |
120 |
 |
| 21.40–21.70 | 40 |
 |
353 |
 |
| 21.70–22.00 | 105 |
 |
811 |
 |
| 22.00–22.30 | 171 |
 |
1459 |
 |
| 22.30–22.60 | 268 |
 |
1935 |
 |
| 22.60–22.90 | 332 |
 |
1896 |
 |
| 22.90–23.20 | 276 |
 |
1114 |
 |
| 23.20–23.50 | 251 |
 |
487 |
 |
| 23.50–23.80 | 151 |
 |
165 |
 |
| 23.80–24.10 | 118 |
 |
38 |
 |
| 24.10–24.40 | 81 |
 |
14 |
 |
| 24.40–24.70 | 83 |
 |
||
| 24.70–25.00 | 75 |
 |
||
| 25.00–25.30 | 48 |
 |
||
| 25.30–25.60 | 34 |
 |
||
| 25.60–25.90 | 19 |
 |
||
| 25.90–26.20 | 14 |
 |
||
| 26.20–26.50 | 6 |
 |
||
| 26.50–26.80 | 3 |
 |
||
Notes. The columns show the range of 150 MHz radio luminosities considered in each bin, the total number of radio AGN in that bin, the derived space density of these (in units of number per log10L per Mpc3), the total number of SFGs and their space density. Uncertainties are statistical Poissonian uncertainties only.
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