Table 1.
Main properties of the 3C subsample observed with MUSE.
| Name | z | Class | Lbol | Seeing | Scale |
|---|---|---|---|---|---|
| [erg s−1] | ″ | kpc/1″ | |||
| 3C 015 | 0.073 | LEG | 43.39 | 0.65 | 1.39 |
| 3C 017 | 0.22 | BLO | 44.77 | 0.49 | 3.55 |
| 3C 018 | 0.188 | BLO | 45.34 | 0.53 | 3.14 |
| 3C 029 | 0.045 | LEG | 42.88 | 0.51 | 0.88 |
| 3C 033 | 0.06 | HEG | 44.97 | 0.63 | 1.16 |
| 3C 040 | 0.018 | LEG | 41.99 | 0.40 | 0.37 |
| 3C 063 | 0.175 | HEG | 44.42 | 0.49 | 2.97 |
| 3C 076.1 | 0.032 | – | 42.61 | 0.62 | 0.64 |
| 3C 078 | 0.028 | LEG | 42.18 | 0.53 | 0.56 |
| 3C 079 | 0.256 | HEG | 45.64 | 0.66 | 3.98 |
| 3C 088 | 0.03 | LEG | 42.92 | 0.59 | 0.60 |
| 3C 089 | 0.138 | – | 43.29 | 0.64 | 2.44 |
| 3C 098 | 0.03 | HEG | 43.78 | 0.66 | 0.60 |
| 3C 105 | 0.089 | HEG | 44.24 | 0.71 | 1.66 |
| 3C 135 | 0.125 | HEG | 44.83 | 0.52 | 2.24 |
| 3C 180 | 0.22 | HEG | 45.12 | 1.45 | 3.55 |
| 3C 196.1 | 0.198 | LEG | 44.31 | 0.48 | 3.27 |
| 3C 198 | 0.081 | SF | 43.76 | 0.78 | 1.53 |
| 3C 227 | 0.086 | BLO | 44.55 | 0.91 | 1.61 |
| 3C 264 | 0.021 | LEG | 41.95 | 0.85 | 0.43 |
| 3C 272 | 0.003 | LEG | 40.78 | 0.39 | 0.06 |
| 3C 287.1 | 0.216 | BLO | 44.53 | 0.65 | 3.50 |
| 3C 296 | 0.024 | LEG | 42.52 | 1.08 | 0.48 |
| 3C 300 | 0.27 | HEG | 44.79 | 0.41 | 4.14 |
| 3C 327 | 0.105 | HEG | 45.03 | 0.70 | 1.93 |
| 3C 348 | 0.155 | LEG | 43.20 | 1.76 | 2.69 |
| 3C 353 | 0.03 | LEG | 42.92 | 1.30 | 0.60 |
| 3C 403 | 0.059 | HEG | 44.54 | 0.54 | 1.14 |
| 3C 403.1 | 0.055 | LEG | 42.64 | 0.80 | 1.07 |
| 3C 424 | 0.127 | LEG | 43.59 | 0.98 | 2.27 |
| 3C 442 | 0.026 | LEG | 42.00 | 0.61 | 0.52 |
| 3C 445 | 0.056 | BLO | 45.28 | 1.48 | 1.09 |
| 3C 456 | 0.233 | HEG | 45.60 | 1.27 | 3.71 |
| 3C 458 | 0.289 | HEG | 44.82 | 0.50 | 4.34 |
| 3C 459 | 0.22 | BLO | 44.82 | 0.43 | 3.55 |
Notes. Column description: (1) source name; (2) redshift; (3) excitation class (in some cases, the strength of the emission lines is insufficient for a robust spectroscopic classification) from Buttiglione et al. (2010); (4) AGN bolometric luminosity obtained by applying a bolometric correction of 600 to the absorption-corrected nuclear [O III] luminosity; (5) mean seeing of the observation; (6) conversion factor from arcsec into kpc.
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