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Table 1.

Sample properties.

Name Redshift FR Exc. Radio
 Line emission
 Kinemetry Host
class PA LAS PA (1) PA (2) r (kpc) PA PA
3C 015 0.073 I LEG 152 59 [N II] 120 0 6.7 – 20
3C 017 0.220 II BLO 156 49 [N II] 280 11.6 – 0
3C 018 0.188 II BLO 163 167 [O III] 50 270 20.1 – 165
3C 029 0.045 I LEG 160 115 [O III] – 100
3C 033 0.060 II HEG 19 313 [O III] 70 270 10.7 80 165
3C 040 0.018 I LEG 13 450 [N II] – 100
3C 063 0.175 II HEG 33 53 Hα 260 90 31.5 – 75
3C 076.1 0.032 I – 130 106 [N II] 50 270 4.2 110 130
3C 078 0.028 I LEG 53 39 [N II] 80 155
3C 079 0.256 II HEG 105 537 [O III] 160 330 35.7 0 15
3C 088 0.030 II LEG 55 107 [N II] 90 3.7 120 150
3C 089 0.138 I – 120 161 [N II] 300 8.8 – 40
3C 098 0.030 II HEG 25 145 [O III] 350 170 16.3 5 55
3C 105 0.089 II HEG 127 131 [O III] 10 50
3C 135 0.125 II HEG 75 216 [O III] 230 50 43.7 30 130
3C 180 0.220 II HEG 10 3080 [O III] 40 210 34.9 35 30
3C 196.1 0.198 II LEG 45 63 [O III] 60 14.5 – 50
3C 198 0.081 II SF 30 117 Hα 220 35.2 0 65
3C 227 0.086 II BLO 85 514 [O III] 50 220 49.6 120 0
3C 264 0.021 I LEG 120 68 [N II] 145 15
3C 272.1 0.003 I LEG 175 5 [N II] 80 260 0.5 80 130
3C 287.1 0.216 II BLO 90 283 [O III] 170 40 27.0 100 30
3C 296 0.024 I LEG 35 130 [N II] – 145
3C 300 0.270 II HEG 132 374 [O III] 130 260 36.3 85 125
3C 318.1 0.045 – – [N II] 190 18.1 – 105
3C 327 0.105 II HEG 100 489 [N II] 170 20 16.3 45 135
3C 348 0.155 I ELEG 36 545 Hα 280 110 28.2 0 145
3C 353 0.030 II LEG 82 125 Hα 0 180 15.4 – 75
3C 386 0.017 II – 16 88 [N II] 80 270 10.1 130 105
3C 403 0.059 II HEG 86 110 [O III] 200 30 8.7 35 40
3C 403.1 0.055 II LEG 127 260 Hα 230 50 5.3 20 150
3C 424 0.127 II LEG 155 28 [N II] 130 29.0 80 80
3C 442 0.026 II LEG 63 322 [N II] 190 4.1 120 130
3C 445 0.056 II BLO 173 532 [O III] 235 105 15.7 – –
3C 456 0.233 II HEG 17 21 [O III] 120 –
3C 458 0.289 II HEG 75 804 [O III] 30 220 81.2 20 55
3C 459 0.220 II BLO 97 28 [O III] 320 59.6 120 –

Notes. Column description: (1) source name; (2) redshift; (3) and (4) radio morphological classification and excitation class from Buttiglione et al. (2010) (LEG = low excitation galaxy, HEG = high excitation galaxy, BLO = broad line object, SF = star-forming galaxy, ELEG = extremely low excitation galaxy); (5) and (6) position angle and largest angular size of the radio source with uncertainties usually between 5° and 10°; (7)–(9) emission line considered and position angles of the ionized gas on each side of the nucleus, (10) largest distance of emission line detection, (11) perpendicular to the line of nodes derived with the kinemetry software (kinematical axis), (12) host position angle.

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