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Table 1.
Eddington ratios from radiative luminosity, not corrected for redshift dependence.
| Radio | N | Log10(λr) |
Log10(LX/Lradio) |
|||||
|---|---|---|---|---|---|---|---|---|
| class | Median | 16% | 84% | Median | 16% | 84% | ||
| FRII | Detected | 18 | −2.20 | −2.27 | −2.11 | 1.76 | 1.72 | 1.81 |
| Stacked | 30 | −3.43 | −3.55 | −3.30 | 1.00 | 0.87 | 1.13 | |
| FRI | Detected | 6 | −1.82 | −1.90 | −1.74 | 2.64 | 2.58 | 2.71 |
| Stacked | 25 | < −3.52 | − | − | < 1.65 | − | − | |
| FRI/FRII | Detected | 8 | −2.43 | −2.52 | −2.26 | 1.88 | 1.83 | 1.92 |
| Stacked | 12 | −3.19 | −3.37 | −3.00 | 1.62 | 1.44 | 1.81 | |
| COM AGN | Detected | 291 | −1.96 | −1.99 | −1.94 | 3.47 | 3.45 | 3.49 |
| Stacked | 1386 | −3.22 | −3.35 | −3.08 | 2.35 | 2.21 | 2.49 | |
Notes. Eddington ratios using radiative luminosity, λr = Lrad/LEdd (see Sect. 3.2). The 16th and 84th percentile values indicate uncertainties on the medians.
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