Table 31.
Radio-loudness parameters and ionisation ratios.
| ID | log(L5100) | log(L5100) | log(L1.4 GHz) | R1.4/5100 | R1.4/5100 | log([O III]λ5007/Hβ) |
|---|---|---|---|---|---|---|
| (*-non-radio) | (SDSS) | (LBT) | (SDSS) | (LBT) | ||
| H011A | 39.461 | 38.883 | 40.232 | 5.895 | 22.343 | 0.04279 |
| L024A | 39.375 | 39.489 | 39.642 | 1.847 | 1.420 | 0.23394 |
| L084B | 39.116 | 38.545 | 38.912 | 0.625 | 2.331 | 0.17938 |
| L097A | 39.453 | 38.688 | 38.971 | 0.329 | 1.919 | −0.74123 |
| L115B | 39.295 | 38.556 | 39.462 | 1.470 | 8.048 | −0.22287 |
| L125B | 39.330 | 38.937 | 39.134 | 0.637 | 1.566 | −0.08857 |
| L127B | 39.115 | 38.584 | 39.247 | 1.355 | 4.601 | −0.16620 |
| L156A | 39.244 | 38.705 | 39.228 | 0.963 | 3.333 | 0.17341 |
| L170B | 39.418 | 38.678 | 39.216 | 0.627 | 3.448 | 0.19210 |
| Median | 0.963 | 3.333 | 0.04279 | |||
| Mean | 1.528 | 5.445 | ||||
| H011B* | NA | 38.786 | < 39.176 | NA | < 2.780 | 0.01566 |
| L024B* | NA | 39.396 | < 38.623 | NA | < 0.173 | 0.37143 |
| L084A* | 38.871 | 38.373 | < 37.903 | < 0.109 | < 0.343 | 0.45647 |
| L097B* | 38.567 | 38.007 | < 38.363 | < 0.633 | < 2.300 | 0.23130 |
| L115A | NA | 39.015 | ∼38.948 | NA | ∼0.857 | −0.27613 |
| L115C* | 39.088 | 38.646 | < 38.431 | < 0.163 | < 0.451 | 0.51952 |
| L125A* | NA | 38.101 | < 38.079 | NA | < 0.792 | 0.65003 |
| L127A* | 38.941 | 38.41 | < 38.208 | < 0.114 | < 0.389 | −0.53865 |
| L127C* | 38.431 | 37.957 | < 38.204 | < 0.371 | < 1.104 | 0.41516 |
| L156B* | NA | 39.025 | < 38.751 | NA | < 0.532 | −0.64749 |
| L170A | 38.583 | 38.111 | ∼38.965 | < 2.410 | ∼7.147 | −0.13643 |
| Median | 0.267 | 0.792 | 0.01566 | |||
| Mean | 0.633 | 1.533 | ||||
| RLBT/RSDSS | ||||||
| Median | 3.46 | |||||
| Mean | 3.56 |
Notes. Continuum luminosities at 5100 Å corresponding to the SDSS and LBT spectra, radio luminosity at 1.4 GHz, radio-loudness parameters estimated using the SDSS and LBT continuum luminosities, and the log([O III]λ5007/Hβ) ionisation ratios for all of the galaxies in our sample. ‘NA’ is used as the placeholder for galaxies that do not have a published SDSS spectrum. Luminosities are quoted in units of ergs s−1.
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