Best-fit parameters for log(|$\xi _{\rm {ion},0}$|)-M|$_{\rm {UV}}$| relations, with form log(|$\xi _{\rm {ion},0}$|)|$= \alpha$|M|$_{\rm {UV}}+$|log(|$\xi _{\rm {ion}}$||$_{\rm {,int}}$|) shown in Fig. 9, where |$\xi _{\rm {ion}}$||$_{\rm {,int}}$| is the intercept of the relation. Column 1: redshift bin. Column 2,3: slope and |$\xi _{\rm {ion},0}$| normalisation for the star-forming (SF) sample. Column 4,5: slope and |$\xi _{\rm {ion},0}$| normalisation for the mini-quenched (MQ) sample. For |$z\ge 7$| we only provide relations for the star-forming sample, since there are not enough mini-quenched galaxies to obtain a reliable fit.
| Redshift . | |$\alpha$| . | log(|$\xi _{\rm {ion}}$||$_{,0}$|/[Hz erg|$^{-1}$|]) . | |$\alpha$| . | log(|$\xi _{\rm {ion}}$||$_{,0}$|/[Hz erg|$^{-1}$|]) . |
|---|---|---|---|---|
| . | [SF] . | [SF] . | [MQ] . | [MQ] . |
| |$3 \le z \le 4$| | |$-0.01\pm 0.00$| | |$25.20\pm 0.07$| | |$-0.06\pm 0.06$| | |$23.23\pm 1.04$| |
| |$4 \lt z \le 5$| | |$-0.02\pm 0.01$| | |$24.89\pm 0.11$| | |$-0.02\pm 0.04$| | |$23.95\pm 0.76$| |
| |$5 \lt z \le 6$| | |$-0.05\pm 0.01$| | |$24.32\pm 0.12$| | |$0.03\pm 0.04$| | |$24.74\pm 0.67$| |
| |$6 \lt z \le 7$| | |$-0.03\pm 0.02$| | |$24.88\pm 0.27$| | |$0.01\pm 0.04$| | |$24.51\pm 0.77$| |
| |$7 \lt z \le 8$| | |$-0.05\pm 0.02$| | |$24.51\pm 0.32$| | -- | -- |
| |$8 \lt z \le 9$| | |$-0.12\pm 0.05$| | |$23.28\pm 0.94$| | -- | -- |
| Redshift . | |$\alpha$| . | log(|$\xi _{\rm {ion}}$||$_{,0}$|/[Hz erg|$^{-1}$|]) . | |$\alpha$| . | log(|$\xi _{\rm {ion}}$||$_{,0}$|/[Hz erg|$^{-1}$|]) . |
|---|---|---|---|---|
| . | [SF] . | [SF] . | [MQ] . | [MQ] . |
| |$3 \le z \le 4$| | |$-0.01\pm 0.00$| | |$25.20\pm 0.07$| | |$-0.06\pm 0.06$| | |$23.23\pm 1.04$| |
| |$4 \lt z \le 5$| | |$-0.02\pm 0.01$| | |$24.89\pm 0.11$| | |$-0.02\pm 0.04$| | |$23.95\pm 0.76$| |
| |$5 \lt z \le 6$| | |$-0.05\pm 0.01$| | |$24.32\pm 0.12$| | |$0.03\pm 0.04$| | |$24.74\pm 0.67$| |
| |$6 \lt z \le 7$| | |$-0.03\pm 0.02$| | |$24.88\pm 0.27$| | |$0.01\pm 0.04$| | |$24.51\pm 0.77$| |
| |$7 \lt z \le 8$| | |$-0.05\pm 0.02$| | |$24.51\pm 0.32$| | -- | -- |
| |$8 \lt z \le 9$| | |$-0.12\pm 0.05$| | |$23.28\pm 0.94$| | -- | -- |
Best-fit parameters for log(|$\xi _{\rm {ion},0}$|)-M|$_{\rm {UV}}$| relations, with form log(|$\xi _{\rm {ion},0}$|)|$= \alpha$|M|$_{\rm {UV}}+$|log(|$\xi _{\rm {ion}}$||$_{\rm {,int}}$|) shown in Fig. 9, where |$\xi _{\rm {ion}}$||$_{\rm {,int}}$| is the intercept of the relation. Column 1: redshift bin. Column 2,3: slope and |$\xi _{\rm {ion},0}$| normalisation for the star-forming (SF) sample. Column 4,5: slope and |$\xi _{\rm {ion},0}$| normalisation for the mini-quenched (MQ) sample. For |$z\ge 7$| we only provide relations for the star-forming sample, since there are not enough mini-quenched galaxies to obtain a reliable fit.
| Redshift . | |$\alpha$| . | log(|$\xi _{\rm {ion}}$||$_{,0}$|/[Hz erg|$^{-1}$|]) . | |$\alpha$| . | log(|$\xi _{\rm {ion}}$||$_{,0}$|/[Hz erg|$^{-1}$|]) . |
|---|---|---|---|---|
| . | [SF] . | [SF] . | [MQ] . | [MQ] . |
| |$3 \le z \le 4$| | |$-0.01\pm 0.00$| | |$25.20\pm 0.07$| | |$-0.06\pm 0.06$| | |$23.23\pm 1.04$| |
| |$4 \lt z \le 5$| | |$-0.02\pm 0.01$| | |$24.89\pm 0.11$| | |$-0.02\pm 0.04$| | |$23.95\pm 0.76$| |
| |$5 \lt z \le 6$| | |$-0.05\pm 0.01$| | |$24.32\pm 0.12$| | |$0.03\pm 0.04$| | |$24.74\pm 0.67$| |
| |$6 \lt z \le 7$| | |$-0.03\pm 0.02$| | |$24.88\pm 0.27$| | |$0.01\pm 0.04$| | |$24.51\pm 0.77$| |
| |$7 \lt z \le 8$| | |$-0.05\pm 0.02$| | |$24.51\pm 0.32$| | -- | -- |
| |$8 \lt z \le 9$| | |$-0.12\pm 0.05$| | |$23.28\pm 0.94$| | -- | -- |
| Redshift . | |$\alpha$| . | log(|$\xi _{\rm {ion}}$||$_{,0}$|/[Hz erg|$^{-1}$|]) . | |$\alpha$| . | log(|$\xi _{\rm {ion}}$||$_{,0}$|/[Hz erg|$^{-1}$|]) . |
|---|---|---|---|---|
| . | [SF] . | [SF] . | [MQ] . | [MQ] . |
| |$3 \le z \le 4$| | |$-0.01\pm 0.00$| | |$25.20\pm 0.07$| | |$-0.06\pm 0.06$| | |$23.23\pm 1.04$| |
| |$4 \lt z \le 5$| | |$-0.02\pm 0.01$| | |$24.89\pm 0.11$| | |$-0.02\pm 0.04$| | |$23.95\pm 0.76$| |
| |$5 \lt z \le 6$| | |$-0.05\pm 0.01$| | |$24.32\pm 0.12$| | |$0.03\pm 0.04$| | |$24.74\pm 0.67$| |
| |$6 \lt z \le 7$| | |$-0.03\pm 0.02$| | |$24.88\pm 0.27$| | |$0.01\pm 0.04$| | |$24.51\pm 0.77$| |
| |$7 \lt z \le 8$| | |$-0.05\pm 0.02$| | |$24.51\pm 0.32$| | -- | -- |
| |$8 \lt z \le 9$| | |$-0.12\pm 0.05$| | |$23.28\pm 0.94$| | -- | -- |
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