Table B.1.
Average corrections of luminosity at 1.4 GHz needed if the K-correction was performed by assuming a power-law SED with a spectral index of 0.7.
| z | CL1.4 GHz (logCL1.4 GHz (dex)) | ||||
|---|---|---|---|---|---|
| p< 10 | |||||
| 0% | 25% | 50% | 75% | 100% | |
| 0.0 | 0.81 (−0.09) | 0.89 (−0.05) | 0.97 (−0.02) | 1.04 (0.02) | 1.12 (0.05) |
| 0.5 | 0.74 (−0.13) | 0.85 (−0.07) | 0.95 (−0.02) | 1.06 (0.02) | 1.17 (0.07) |
| 1.0 | 0.79 (−0.10) | 0.89 (−0.05) | 0.99 (−0.01) | 1.08 (0.03) | 1.18 (0.07) |
| 1.5 | 0.83 (−0.08) | 0.92 (−0.04) | 1.01 (0.00) | 1.10 (0.04) | 1.18 (0.07) |
| 2.0 | 0.87 (−0.06) | 0.95 (−0.02) | 1.02 (0.01) | 1.10 (0.04) | 1.18 (0.07) |
| 2.5 | 0.90 (−0.04) | 0.97 (−0.01) | 1.04 (0.02) | 1.10 (0.04) | 1.17 (0.07) |
| 3.0 | 0.93 (−0.03) | 0.99 (−0.00) | 1.04 (0.02) | 1.10 (0.04) | 1.15 (0.06) |
| 3.5 | 0.96 (−0.02) | 1.01 (0.00) | 1.05 (0.02) | 1.09 (0.04) | 1.14 (0.06) |
| 4.0 | 0.99 (−0.01) | 1.02 (0.01) | 1.06 (0.02) | 1.09 (0.04) | 1.12 (0.05) |
Notes.
The corrections were derived for the average luminosity at 1.4 GHz, as described in Sect. B, and are based on the assumption that galaxies with an SFR > 10 M⊙ yr−1 follow the broken power-law (BPL) SED and that galaxies with an SFR < 10 M⊙ yr−1 follow the SED based on Eq. (2), with the nonthermal spectral index and thermal fraction taken from Tabatabaei et al. (2017). The percentage p< 10 is the percentage of 3 GHz flux that is due to galaxies with an SFR < 10 M⊙ yr−1. Columns of p< 10 = 0% and p< 10 = 100% are also exact corrections for single objects derived by assuming the BPL or the Tabatabaei et al. (2017) SEDs, respectively. The values in parentheses are correction CL1.4 GHz expressed in dex.
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