Table 7
Best-fit values for each frequency, as well as the reduced χ2.
| Frequency (GHz) | log 10Mmin [h-1 M⊙] | αsat | jeff [Jy/Mpc/sr] | Reduced χ2 (χ2 / d.o.f.) |
|
|
||||
| 217 | 11.95 ± 2.10 | 1.30 ± 1.16 | 7.51 ± 0.75 × 101 | 2.68 (16.1/6) |
| 353 | 12.49 ± 0.42 | 1.39 ± 0.42 | 2.00 ± 0.29 × 102 | 2.42 (14.5/6) |
| 545 | 12.35 ± 1.01 | 1.17 ± 0.65 | 3.11 ± 3.85 × 102 | 0.50 (3.04/6) |
| 857 | 12.20 ± 0.51 | 1.02 ± 0.87 | 3.14 ± 17.0 × 102 | 0.73 (4.40/6) |
| 217 | 11.82 ± 1.92 | 1.17 ± 2.38 | N/A | 1.14 (7.96/7) |
| 353 | 12.50 ± 0.09 | 1.35 ± 0.20 | N/A | 0.80 (5.64/7) |
| 545 | 12.35 ± 0.94 | 1.17 ± 0.45 | N/A | 0.35 (2.46/7) |
| 857 | 12.21 ± 1.23 | 0.96 ± 0.73 | N/A | 0.60 (4.22/7) |
Notes. The errors correspond to the 1σ Gaussian errors, including statistical and photometric calibration systematic contributions. Systematic errors introduced by the beam uncertainty (see Sect. 4.2.2) are not included here, but contribute less than an extra 10% to the error budget. The upper half of the array allows for a freely varying jeff per frequency, while in the bottom half jeff is fixed to the extrapolation coming from our model.
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