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Table 1.

Main properties of the 3C subsample observed with MUSE, and the observations log.

Name z FR Class L178 r L[NII],nuc L[NII],ext LHα, nuc LHα, ext L[OIII],nuc L[OIII],ext Obs. date Seeing Sky Depth
3C 015 0.073 I LEG 33.30 6.7 40.91 40.24 40.23 38.16 40.51 38.16 Jun 30 2017 0.65 TN 5.6
3C 017 0.220 II BLO 34.44 11.6 41.95 41.25 42.15 42.58 41.86 41.41 Jul 20 2017 0.49 TN/CL 5.9
3C 018 0.188 II BLO 34.27 20.1 41.74 41.17 41.61 41.17 42.14 41.46 Jun 30 2017 0.53 TN 5.9
3C 029 0.045 I LEG 32.84 < 1.4 40.39 < 39.91 39.73 38.75 39.81 38.38 Jul 20 2017 0.51 TN/CL 3.2
3C 033 0.060 II HEG 33.65 10.7 41.04 41.02 41.18 41.32 41.66 41.75 Jun 30 2017 0.63 TN 7.4
3C 040 0.018 I LEG 32.29 < 0.5 39.65 < 38.42 39.38 38.22 39.0 37.13 Jul 22 2017 0.40 TN/CL 7.5
3C 063 0.175 II HEG 34.21 31.5 40.95 41.05 41.31 41.48 41.41 40.98 Jul 21 2017 0.49 TN 7.5
3C 076.1 0.032 I – 32.46 4.2 39.63 39.36 38.97 37.46 39.84 < 38.22 Jan 05 2019 0.62 TN 1.9
3C 078 0.028 I LEG 32.51 < 0.9 40.34 < 39.84 39.7 < 38.82 39.41 < 38.82 Nov 11 2018 0.53 TN 10.1
3C 079 0.256 II HEG 34.78 35.7 40.09 41.89 42.49 42.59 42.93 42.91 Jan 05 2019 0.66 TN 4.8
3C 088 0.030 II LEG 32.49 3.7 40.38 39.75 40.38 40.06 39.88 39.12 Nov 11 2018 0.59 TN/CL 1.7
3C 089 0.138 I – 34.01 8.8 40.39 39.67 39.47 38.62 40.52 < 39.76 Dec 29 2018 0.64 TN 3.1
3C 098 0.030 II HEG 32.99 16.3 40.20 40.03 40.29 40.46 40.75 40.75 Nov 05 2018 0.66 TN 0.5
3C 105 0.089 II HEG 33.54 < 3.6 40.85 < 40.15 40.63 39.89 41.01 40.39 Dec 30 2018 0.71 TN/CL 8.4
3C 135 0.125 II HEG 33.84 43.7 41.38 40.78 41.44 41.12 41.95 41.42 Dec 06 2018 0.52 TN 3.2
3C 180 0.220 II HEG 34.32 34.9 40.93 41.68 41.82 42.14 42.35 42.66 Dec 03 2018 1.45 CL 3.6
3C 196.1 0.198 II LEG 34.31 14.5 41.36 41.66 41.22 41.6 41.3 41.05 Jan 13 2019 0.48 TN 1.1
3C 198 0.081 II SF 33.19 35.2 40.85 40.41 41.38 41.14 41.07 41.32 Jan 14 2019 0.78 TN 1.1
3C 227 0.086 II BLO 33.74 49.6 41.15 41.27 41.61 41.74 41.82 42.13 Jan 28 2019 0.91 TN/CL 1.1
3C 264 0.021 I LEG 32.43 < 1.1 40.01 < 39.28 39.79 39.34 39.15 37.18 Jan 12 2019 0.85 TN 1.7
3C 272.1 0.003 I LEG 30.72 0.5 38.98 39.45 38.78 39.44 38.45 39.27 Feb 03 2019 0.39 TN 17.5
3C 287.1 0.216 II BLO 34.04 27.0 41.47 41.94 41.59 41.18 41.88 41.47 Jun 30 2018 0.65 TN 7.1
3C 296 0.024 I LEG 32.22 < 1.6 40.09 < 39.20 39.67 38.44 39.58 38.37 Feb 11 2019 1.08 TN/CL 1.3
3C 300 0.270 II HEG 34.60 36.3 41.12 40.61 41.87 42.37 42.3 42.78 Mar 11 2019 0.41 TN 4.1
3C 318.1 0.045 – – 32.72 18.1 39.91 40.71 38.95 40.16 39.40 < 39.03 Jun 22 2017 1.38 CL 6.3
3C 327 0.105 II HEG 33.98 16.3 41.67 40.97 41.79 40.98 41.67 40.97 Jun 30 2017 0.70 TN 6.3
3C 348 0.155 I ELEG 35.35 28.2 41.32 42.33 41.18 41.12 40.09 39.69 Jul 20 2017 1.76 CL 3.5
3C 353 0.030 II LEG 33.69 15.4 40.04 39.70 40.0 39.84 39.54 39.28 Jun 29 2017 1.30 CL 4.1
3C 386 0.017 II – 32.18 10.1 39.51 40.26 39.22 40.25 40.22 < 38.23 Jun 03 2017 0.61 TN 7.3
3C 403 0.059 II HEG 33.16 8.7 40.82 41.69 40.87 40.83 41.33 41.71 Jun 30 2017 0.54 TN 5.5
3C 403.1 0.055 II LEG 32.98 5.3 39.83 40.20 39.78 40.59 39.51 40.18 Jun 30 2017 0.80 TN 4.5
3C 424 0.127 II LEG 33.78 29.0 40.70 41.45 40.75 41.67 40.27 41.0 Jul 01 2017 0.98 TN 1.2
3C 442 0.026 II LEG 32.39 4.1 39.92 40.11 39.56 39.54 39.16 38.9 Jun 30 2017 0.61 TN 11.3
3C 445 0.056 II BLO 33.26 15.7 42.20 41.12 42.5 42.02 42.2 41.87 Jul 01 2017 1.48 TN/CL 5.2
3C 456 0.233 II HEG 34.23 < 14.3 42.46 < 41.78 42.57 41.74 42.88 42.11 Jun 30 2017 1.27 TN 8.8
3C 458 0.289 II HEG 34.58 81.2 40.96 40.84 41.12 41.67 41.64 42.09 Jul 22 2017 0.50 TN/CL 5.6
3C 459 0.220 II BLO 34.55 59.6 42.39 41.87 42.15 41.83 41.83 42.02 Jul 22 2017 0.43 TN/CL 19.3

Notes. Column description: (1) Name: source name. The 17 newly observed sources are shown in boldface; (2) z: redshift; (3 and 4) FR and excitation class from Buttiglione et al. (2010, 2011). We used their criterion for the HERG/LERG separation; some sources lack a spectral classification due to the non-detection of the key diagnostic emission lines; (5) L178: radio luminosity at 178 MHz in erg s−1 Hz−1, from Spinrad et al. (1985); (6) r: largest distance of emission line detection in kpc units; (from 7 to 12) Nuclear luminosity and luminosity of the ELR (within three times the seeing of the observations) for [N II], Hα and [O III] all in erg s−1 units; (13) Obs. date: date of the observation; (14) Seeing: mean seeing of the observation; (15) Sky conditions: (TN) thin cirrus clouds, (CL) clear night; (16) Depth: surface brightness limit of emission lines at 3σ in units of 10−18 erg s−1 cm−2 arcsec−2.

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