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Table 6.
Exponents of the SFR–radio correlation.
| ν = 1.4 GHz | Exponent | SFR | Sample |
|---|---|---|---|
| Bell (2003) | 1.3 (Lrad < 6.4 × 1021 L⊙) | Ext-corr Hα | |
| Bell (2003) | 1.0 (Lrad > 6.4 × 1021 L⊙) | Ext-corr Hα | |
| Murphy et al. (2011) | 1.0 | IR | High-z galaxies included |
| Heesen et al. (2014) | 1.11 ± 0.08 | 24 μm + FUV | Ṁ∗ ≲ 10 M⊙ yr−1 |
| Boselli et al. (2015) | 1.18 | Ext-corr Hα | Ṁ∗ ≲ 10 M⊙ yr−1 |
| Brown et al. (2017) | 1.27 ± 0.03 | Ext-corr Hα | Ṁ∗ ≲ 10 M⊙ yr−1 |
| Gürkan et al. (2018) | 0.87 ± 0.01 | SED fitting | Ṁ∗ ≲ 10 M⊙ yr−1 |
| Model (all samples) | 1.05 ± 0.04 | ||
| ν = 150 MHz | |||
| Gürkan et al. (2018) | 1.07 ± 0.01 | SED fitting | Ṁ∗ ≲ 10 M⊙ yr−1 |
| Wang et al. (2019) | 1.35 ± 0.06 | Ext-corr Hα | |
| Smith et al. (2021) | 1.04 ± 0.01 | SED fitting | |
| Model (all samples) | 0.99 ± 0.05 | ||
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