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Table 2.
Eddington ratios from radiative luminosity and Qjet, not corrected for redshift dependence.
| Radio | N | Log10(λrk) |
Log10(LX/Lradio) |
|||||
|---|---|---|---|---|---|---|---|---|
| class | Median | 16% | 84% | Median | 16% | 84% | ||
| FRII | Detected | 18 | −1.13 | −1.15 | −1.10 | 1.76 | 1.71 | 1.81 |
| Stacked | 30 | −1.65 | −1.65 | −1.64 | 1.00 | 0.87 | 1.13 | |
| FRI | Detected | 6 | −1.50 | −1.56 | −1.43 | 2.64 | 2.58 | 2.71 |
| Stacked | 25 | < −2.21 | − | − | < 1.67 | − | − | |
| FRI/FRII | Detected | 8 | −1.32 | −1.40 | −1.28 | 1.88 | 1.83 | 1.93 |
| Stacked | 12 | −1.91 | −1.92 | −1.89 | 1.65 | 1.45 | 1.85 | |
| COM AGN | Detected | 291 | −1.79 | −1.82 | −1.77 | 3.47 | 3.45 | 3.49 |
| Stacked | 1386 | −2.35 | −2.37 | −2.33 | 2.35 | 2.22 | 2.49 | |
Notes. Eddington ratios including radiative luminosity and kinetic energy Qjet, λrk = (Lrad + Qjet)/LEdd (see Sect. 3.2). The 16th and 84th percentile values indicate uncertainties on the medians.
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