Table 1.
Main properties of 3C sub sample observed with MUSE and observations log.
| Name | z | FR | Class | L178 | L.A.S radio | r | Obs. date | Seeing | Weather | Depth |
|---|---|---|---|---|---|---|---|---|---|---|
| [erg s−1 Hz−1] | [kpc] | [kpc] | [″] | |||||||
| 3C 015 | 0.073 | I | LEG | 33.30 | 70 | 1.5 | Jun. 30 2017 | 0.65 | TN | 5.6 |
| 3C 017 | 0.220 | II | BLO | 34.44 | 54 | 14.9 | Jul. 20 2017 | 0.49 | TN/CL | 5.9 |
| 3C 018 | 0.188 | II | BLO | 34.27 | 178 | 24.8 | Jun. 30 2017 | 0.53 | TN | 5.9 |
| 3C 029 | 0.045 | I | LEG | 32.84 | 125 | 0.9 | Jul. 20 2017 | 0.51 | TN/CL | 3.2 |
| 3C 033 | 0.060 | II | HEG | 33.65 | 288 | 11.2 | Jun. 30 2017 | 0.63 | TN | 7.4 |
| 3C 040 | 0.018 | I | LEG | 32.29 | 440 | 1.2 | Jul. 22 2017 | 0.40 | TN/CL. | 7.5 |
| 3C 063 | 0.175 | II | HEG | 34.21 | 56 | 38.0 | Jul. 21 2017 | 0.49 | TN | 7.5 |
| 3C 318.1 | 0.045 | – | – | 32.72 | Jun. 22 2017 | 1.38 | CL | 6.3 | ||
| 3C 327 | 0.105 | II | HEG | 33.98 | 469 | 19.5 | Jun. 30 2017 | 0.70 | TN | 6.3 |
| 3C 348 | 0.155 | I | ELEG | 35.35 | 153 | 34.0 | Jul. 20 2017 | 1.76 | CL | 3.5 |
| 3C 353 | 0.030 | II | LEG | 33.69 | 111 | 17.2 | Jun. 29 2017 | 1.30 | CL | 4.1 |
| 3C 386 | 0.017 | II | – | 32.18 | 77 | 11.1 | Jun. 03 2017 | 0.61 | TN | 7.3 |
| 3C 403 | 0.059 | II | HEG | 33.16 | 101 | 8.3 | Jun. 30 2017 | 0.54 | TN | 5.5 |
| 3C 403.1 | 0.055 | II | LEG | 32.98 | 236 | 5.6 | Jun. 30 2017 | 0.80 | TN | 4.5 |
| 3C 424 | 0.127 | II | LEG | 33.78 | 28 | 32.9 | Jul. 01 2017 | 0.98 | TN | 1.2 |
| 3C 442 | 0.026 | II | LEG | 32.39 | 286 | 3.8 | Jun. 30 2017 | 0.61 | TN | 11.3 |
| 3C 445 | 0.056 | II | BLO | 33.26 | 483 | 18.5 | Jul. 01 2017 | 1.48 | TN/CL | 5.2 |
| 3C 456 | 0.233 | II | HEG | 34.23 | 24 | Jun. 30 2017 | 1.27 | TN | 8.8 | |
| 3C 458 | 0.289 | II | HEG | 34.58 | 943 | 111.3 | Jul. 22 2017 | 0.50 | TN/CL | 5.6 |
| 3C 459 | 0.220 | II | BLO | 34.55 | 31 | 76.0 | Jul. 22 2017 | 0.43 | TN/CL | 19.3 |
Notes. Column description: (1) source name; (2) redshift; (3) and (4) FR and excitation class; (5) radio luminosity at 178 MHz from Spinrad et al. (1985); (6) largest angular size of the radio source; (7) largest distance of emission line detection in kpc units; (8) date of the observation; (9) mean seeing in the V band at zenith during the observation; (10) sky conditions during the observations: (TN) thin cirrus clouds (CL) clear night; (11) surface brightness limit of emission lines at 3σ in units of 10−18 erg s−1 cm−2 arcsec−2.
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