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Table 2.
3CRR quasar sample.
| Name | log LUV | log λO | αOX | log |
|---|---|---|---|---|
| [erg s−1 Hz−1] | ||||
| (1) | (2) | (3) | (4) | (5) |
| 3C 47 | 30.13 | −1.29 | 1.09 |
8.59 |
| 3C 175 | 31.16 | −0.95 | 1.41 |
9.79 |
| 3C 181 | 31.20 | −0.61 | 1.41 |
|
| 3C 196 | 30.77 | −1.05 | 1.37 |
9.55 |
| 3C 204 | 31.12 | −0.60 | 1.30 |
9.59 |
| 3C 207 | 30.37 | −0.35 | 1.16 |
9.02 |
| 3C 208 | 31.10 | −0.52 | 1.41 |
9.55 |
| 3C 212 | 30.60 | −0.81 | 1.07 |
9.45 |
| 3C 245 | 30.96 | −0.65 | 1.29 |
9.63 |
| 3C 249.1 | 30.50 | −1.02 | 1.41 |
8.97 |
| 3C 254 | 30.72 | −0.79 | 1.35 |
8.96 |
| 3C 263 | 31.20 | −0.12 | 1.53 |
9.68 |
| 3C 268.4 | 31.44 | −0.58 | 1.47 |
10.4 |
| 3C 275.1 | 30.06 | −0.46 | 1.44 |
|
| 3C 334 | 30.59 | −1.33 | 1.34 |
9.20 |
| 3C 380 | 30.95 | −0.17 | 1.27 |
9.51 |
Notes. Col. (1): Source name. Col. (2): UV luminosity at 2500 Å. Col. (3): Eddington ratio λO based on optical-UV flux. Col. (4): Optical to X-ray spectral index αOX. Col. (5): Black hole mass calculated with the luminosity at the H band.
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