Measured properties of the primary SFR-selected samples in Fig. 3. For each redshift and SFR range, we present the sample size, average SFR within the bin, and the corresponding radio luminosity. LH α measurements are converted to SFR following equation (1). Limits on |$L_{\rm {1.4\,GHz}}$| represent 2σ upper limits based on the measured background noise in the 2D median stack.
| SFR(LH α) range – ϕ (|$\text{M}_{\odot }\, \text{yr}^{-1}$|) . | N . | 〈SFR(LH α)〉 (|$\text{M}_{\odot }\, \text{yr}^{-1}$|) . | 〈LH α〉 (|$10^{42} \rm {erg\,s}^{-1}$|) . | |$\left\langle L_{\rm {1.4\,GHz}} \right\rangle$| (|$10^{22} \rm {W\,Hz}^{-1}$|) . |
|---|---|---|---|---|
| 1.4 < z < 1.7 | ||||
| 1 < ϕ ≤ 30 | 14 | 4.2 | 0.8 | <1.8 |
| 30 < ϕ | 6 | 48.8 | 8.8 | 18.1 ± 7.0 |
| 2.0 < z < 2.6 | ||||
| 1 < ϕ ≤ 10 | 10 | 7.3 | 1.3 | <9.1 |
| 10 < ϕ ≤ 30 | 25 | 13.4 | 2.4 | 4.8 ± 2.4 |
| 30 < ϕ ≤ 60 | 17 | 40.0 | 7.2 | 8.0 ± 3.8 |
| 60 < ϕ ≤ 120 | 13 | 85.2 | 15.4 | 14.3 ± 3.3 |
| 120 < ϕ | 8 | 190.4 | 34.4 | 20.4 ± 5.5 |
| SFR(LH α) range – ϕ (|$\text{M}_{\odot }\, \text{yr}^{-1}$|) . | N . | 〈SFR(LH α)〉 (|$\text{M}_{\odot }\, \text{yr}^{-1}$|) . | 〈LH α〉 (|$10^{42} \rm {erg\,s}^{-1}$|) . | |$\left\langle L_{\rm {1.4\,GHz}} \right\rangle$| (|$10^{22} \rm {W\,Hz}^{-1}$|) . |
|---|---|---|---|---|
| 1.4 < z < 1.7 | ||||
| 1 < ϕ ≤ 30 | 14 | 4.2 | 0.8 | <1.8 |
| 30 < ϕ | 6 | 48.8 | 8.8 | 18.1 ± 7.0 |
| 2.0 < z < 2.6 | ||||
| 1 < ϕ ≤ 10 | 10 | 7.3 | 1.3 | <9.1 |
| 10 < ϕ ≤ 30 | 25 | 13.4 | 2.4 | 4.8 ± 2.4 |
| 30 < ϕ ≤ 60 | 17 | 40.0 | 7.2 | 8.0 ± 3.8 |
| 60 < ϕ ≤ 120 | 13 | 85.2 | 15.4 | 14.3 ± 3.3 |
| 120 < ϕ | 8 | 190.4 | 34.4 | 20.4 ± 5.5 |
Measured properties of the primary SFR-selected samples in Fig. 3. For each redshift and SFR range, we present the sample size, average SFR within the bin, and the corresponding radio luminosity. LH α measurements are converted to SFR following equation (1). Limits on |$L_{\rm {1.4\,GHz}}$| represent 2σ upper limits based on the measured background noise in the 2D median stack.
| SFR(LH α) range – ϕ (|$\text{M}_{\odot }\, \text{yr}^{-1}$|) . | N . | 〈SFR(LH α)〉 (|$\text{M}_{\odot }\, \text{yr}^{-1}$|) . | 〈LH α〉 (|$10^{42} \rm {erg\,s}^{-1}$|) . | |$\left\langle L_{\rm {1.4\,GHz}} \right\rangle$| (|$10^{22} \rm {W\,Hz}^{-1}$|) . |
|---|---|---|---|---|
| 1.4 < z < 1.7 | ||||
| 1 < ϕ ≤ 30 | 14 | 4.2 | 0.8 | <1.8 |
| 30 < ϕ | 6 | 48.8 | 8.8 | 18.1 ± 7.0 |
| 2.0 < z < 2.6 | ||||
| 1 < ϕ ≤ 10 | 10 | 7.3 | 1.3 | <9.1 |
| 10 < ϕ ≤ 30 | 25 | 13.4 | 2.4 | 4.8 ± 2.4 |
| 30 < ϕ ≤ 60 | 17 | 40.0 | 7.2 | 8.0 ± 3.8 |
| 60 < ϕ ≤ 120 | 13 | 85.2 | 15.4 | 14.3 ± 3.3 |
| 120 < ϕ | 8 | 190.4 | 34.4 | 20.4 ± 5.5 |
| SFR(LH α) range – ϕ (|$\text{M}_{\odot }\, \text{yr}^{-1}$|) . | N . | 〈SFR(LH α)〉 (|$\text{M}_{\odot }\, \text{yr}^{-1}$|) . | 〈LH α〉 (|$10^{42} \rm {erg\,s}^{-1}$|) . | |$\left\langle L_{\rm {1.4\,GHz}} \right\rangle$| (|$10^{22} \rm {W\,Hz}^{-1}$|) . |
|---|---|---|---|---|
| 1.4 < z < 1.7 | ||||
| 1 < ϕ ≤ 30 | 14 | 4.2 | 0.8 | <1.8 |
| 30 < ϕ | 6 | 48.8 | 8.8 | 18.1 ± 7.0 |
| 2.0 < z < 2.6 | ||||
| 1 < ϕ ≤ 10 | 10 | 7.3 | 1.3 | <9.1 |
| 10 < ϕ ≤ 30 | 25 | 13.4 | 2.4 | 4.8 ± 2.4 |
| 30 < ϕ ≤ 60 | 17 | 40.0 | 7.2 | 8.0 ± 3.8 |
| 60 < ϕ ≤ 120 | 13 | 85.2 | 15.4 | 14.3 ± 3.3 |
| 120 < ϕ | 8 | 190.4 | 34.4 | 20.4 ± 5.5 |
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