Table 6.
Luminosity bins and LF points used in Fig. 13.
| log(L) | log(Φ) | ⟨N⟩ | ⟨Ncorr⟩ | ⟨Vmax⟩ |
|---|---|---|---|---|
| erg s−1 | (Δ(log(L)) = 1)−1 Mpc−3 | Mpc3 | ||
| 2.9 < z < 6.7 | ||||
| 39.00 < 39.63 < 40.25 |  |
2.05 | 8.97 | 124.68 |
| 40.25 < 40.38 < 40.50 |  |
3.52 | 7.04 | 4971.62 |
| 40.50 < 40.63 < 40.75 |  |
9.43 | 24.83 | 10977.19 |
| 40.75 < 40.88 < 41.00 |  |
12.77 | 33.27 | 12063.96 |
| 41.00 < 41.13 < 41.25 |  |
18.68 | 48.11 | 12816.23 |
| 41.25 < 41.38 < 41.50 |  |
23.28 | 48.07 | 12991.31 |
| 41.50 < 41.63 < 41.75 |  |
26.81 | 39.75 | 13926.47 |
| 41.75 < 41.88 < 42.00 |  |
26.15 | 35.60 | 14658.58 |
| 42.00 < 42.13 < 42.25 |  |
18.08 | 21.32 | 15017.49 |
| 42.25 < 42.38 < 42.50 |  |
4.22 | 4.28 | 15696.11 |
| 42.50 < 42.63 < 42.75 |  |
3.94 | 3.95 | 16060.71 |
| 42.75 < 42.88 < 43.00 |  |
3.00 | 3.01 | 16141.73 |
| 2.9 < z < 4.0 | ||||
| 40.00 < 40.25 < 40.50 |  |
1.90 | 4.73 | 4430.41 |
| 40.50 < 40.75 < 41.00 |  |
14.99 | 38.65 | 4145.63 |
| 41.00 < 41.25 < 41.50 |  |
18.37 | 45.65 | 4468.50 |
| 41.50 < 41.75 < 42.00 |  |
14.53 | 18.14 | 5178.73 |
| 42.00 < 42.25 < 42.50 |  |
8.17 | 8.69 | 5216.12 |
| 42.50 < 42.75 < 43.00 |  |
2.95 | 2.95 | 5437.33 |
| 4.0 < z < 5.0 | ||||
| 39.00 < 39.25 < 39.50 |  |
0.76 | 5.47 | 44.11 |
| 39.50 < 40.00 < 40.50 |  |
1.79 | 3.71 | 939.22 |
| 40.50 < 40.75 < 41.00 |  |
4.83 | 14.76 | 2818.30 |
| 41.00 < 41.25 < 41.50 |  |
13.72 | 28.05 | 3706.94 |
| 41.50 < 41.75 < 42.00 |  |
19.40 | 21.96 | 4113.33 |
| 42.00 < 42.25 < 42.50 |  |
8.49 | 8.58 | 4254.24 |
| 42.50 < 42.75 < 43.00 |  |
3.00 | 3.02 | 4430.02 |
| 5.0 < z < 6.7 | ||||
| 40.00 < 40.25 < 40.50 |  |
0.66 | 1.25 | 50.28 |
| 40.50 < 40.75 < 41.00 |  |
2.43 | 4.84 | 2985.57 |
| 41.00 < 41.25 < 41.50 |  |
9.88 | 22.43 | 4763.46 |
| 41.50 < 41.75 < 42.00 |  |
19.06 | 35.27 | 5087.77 |
| 42.00 < 42.25 < 42.50 |  |
5.61 | 8.29 | 5469.76 |
| 42.50 < 42.75 < 43.00 |  |
1.00 | 1.00 | 6187.25 |
Notes. The value ⟨N⟩ is the average number of sources in the luminosity bin and Ncorr is the average number corrected for completeness. The value ⟨Vmax⟩ is the average Vmax for the sources in the bin. The average values are taken across the multiple MC iterations used to compute the statistical errors on the LF points. The uncertainties on log(Φ) are 68% error bars, combining Poissonian error, MC iterations, and an estimation of the cosmic variance.
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