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Table 4

Radio and optical parameters.

Galaxy 2nd component
Source log M/M⊙ age C1a C2b log P FR Spec. L Hα XUV log RW log M/M⊙
109 yr 1033 W mag (BH)
B2 0034+25 11.799 13.0 .. .. 14.4 23.52 1.0 0 .. .. + 0.03 ± .22 1.95 8.87e
B2 0648+27 11.690 13.0 9.620 2.9E8 g 6.8 23.94 3.0 3 S .. .. 0.25 7.49
B2 0755+37 12.102 13.0 .. .. 7.5 24.81 1.5 2 H: 4.65 + 0.34 ± .09 1.79 8.79
B2 0800+24 11.451 13.0 .. .. 6.2 23.83 1.0 1 L: 0.29 .. .. ..
B2 0828+32 11.505 10.0 .. .. 8.2 25.04 2.0 3 L 1.37 −0.3 ± .3 1.56 ..
B2 0836+29 12.036 13.0 .. .. 12.9 24.86 1.5 1 H 2.88 −0.3 ± .4 1.66 ..
B2 0836+29A 11.975 13.0 9.640 2.9E8 g 5.9 25.08 1.5 3 S 25.30 + 1.77 ± .14 0.51 ..
B2 0838+32 11.920 13.0 9.700 5.7E8 g 11.7 24.81 1.0 .. .. .. +1.06 ± .12 1.80 ..
B2 0844+31 12.151 10.0 .. .. 7.6 25.15 1.5 1 L: 2.52 + 0.52 ± .21 1.91 ..
B2 0908+37 12.087 10.0 .. .. 3.3 25.20 1.5 1 L 3.26 −0.3 ± .5 1.91 9.29
B2 0913+38 11.174 5.0 .. .. 2.3 24.62 1.0 1 ? 0.40 + 0.4 ± .5 1.50 ..
B2 0915+32 11.814 13.0 .. .. 1.9 24.34 1.0 1 L: 1.00 + 0.4 ± .3 .. 8.54
B2 0924+30 11.330 5.0 9.750 5.7E8 g 38.3 23.84 1.0 1 A 0.12 + 0.88 ± .02 1.04 8.49
B2 1003+26 12.011 5.0 .. .. 8.0 24.38 .. 1 H 7.36 −0.3 ± .5 1.98 9.51
B2 1005+28 12.000 10.0 9.820 5.7E8 g 13.0 24.64 1.5 0 - <0.48 + 0.34 ± .09 1.73 ..
B2 1037+30 11.660 13.0 9.650 2.9E8 g 7.9 24.87 .. 3 L: 11.70 + 2.53 ± .15 1.22 7.76f
B2 1102+30 11.941 10.0 .. .. 7.7 24.62 1.0 1 A 1.53 + 0.1 ± .4 1.87 ..
B2 1108+27 11.775 13.0 .. .. 15.2 23.62 1.0 1 A 1.45 + 0.43 ± .15 1.56 ..
B2 1113+24 12.168 10.0 .. .. 5.2 24.21 1.0 0 - <0.10 .. .. 9.25
B2 1116+28 11.998 10.0 .. .. 6.7 24.73 1.0 .. .. .. + 0.16 ± .17 2.12 ..
B2 1122+39 11.100 13.0 9.600 1.0E9 g 162.0c 22.11 1.0 2 .. .. + 0.74 ± .03 1.42 7.99e
B2 1141+37 11.580 13.0 8.600 2.9E8 g 18.7c 25.84 2.0 0 .. <0.06 + 1.1 ± .4 1.16 ..
B2 1144+35 11.880 13.0 9.250 2.9E8 g 22.2 24.85 1.0 4 S1 16.74 + 1.68 ± .12 1.07 8.16g
B2 1204+24 11.641 10.0 .. .. 4.9 24.26 1.0 .. .. .. −0.4 ± .3 1.91 ..
B2 1204+34 11.485 5.0 6.800 1.0E6 g 9.5 24.82 2.0 3 S 25.42 + 2.00 ± .08 0.89 8.15
B2 1217+29 10.400 13.0 8.400 5.7E8 g 134.0c 21.54 3.0 2 L .. + 1.64 ± .01 1.83 8.44e
B2 1243+26 11.971 10.0 .. .. 4.1 24.58 1.0 2 L .. + 0.1 ± .3 0.43 ..
B2 1254+27 11.800 13.0 9.700 5.7E8 g 78.0c 22.95 1.0 0 - <0.02 + 1.15 ± .03 1.38 ..
B2 1256+28 11.100 10.0 9.300 1.0E9 g 11.9 23.36 1.0 .. .. .. + 0.43 ± .15 1.91 8.17e
B2 1257+28 11.982 13.0 .. .. 24.5 23.39 1.0 0 - <0.01 + 0.08 ± .12 1.66 8.72e
B2 1300+32 11.755 10.0 .. .. 3.4 25.35 1.0 .. .. .. + 0.9 ± .5 .. ..
B2 1303+31 11.878 5.0 .. .. 10.3 24.80 1.0 .. .. .. + 0.3 ± .8 1.34 ..
B2 1316+29 11.436 5.0 .. .. 3.4 25.17 1.0 1 L 1.28 + 0.2 ± .4 1.25 ..
B2 1317+33 11.700 13.0 .. .. 3.6 23.40 1.0 1 L: 1.20 + 0.34 ± .20 .. ..
B2 1321+31 11.250 10.0 9.750 1.0E9 g 43.9 24.15 1.0 1 L: 0.22 + 0.61 ± .02 1.86 8.08e
B2 1322+36 11.250 10.0 9.750 1.0E9 g 21.0 24.86 1.0 1 L: 0.56 + 0.57 ± .03 1.73 8.59
B2 1339+26 11.250 13.0 9.000 2.9E8 g 13.0c 24.65 1.0 0 - <0.08 + 2.26 ± .21 1.91 9.26
B2 1346+26 12.150 13.0 9.900 2.9E8 g 4.9 24.89 1.0 2 L .. + 1.95 ± .08 1.87 8.86e
B2 1347+28 11.561 10.0 .. .. 8.5 24.40 1.5 1 L: 0.58 + 0.3 ± .3 1.76 8.37
B2 1350+31 11.700 13.0 9.100 2.9E8 g 31.8 25.36 1.5 2 L 6.63 + 1.86 ± .11 0.96 8.15e
B2 1357+28 11.789 13.0 .. .. 5.3 24.37 1.0 .. .. .. −0.1 ± .4 1.92 8.89
B2 1422+26 11.475 10.0 .. .. 2.4 24.32 1.0 3 S 1.72 + 0.30 ± .24 1.45 8.63
B2 1430+25 11.100 5.0 6.700 6.0E6 g 2.6 24.55 1.0 1 L 0.36 + 2.1 ± .3 -0.07 8.17
B2 1447+27 11.552 13.0 .. .. 12.2 23.10 3.0 .. .. .. + 0.46 ± .16 2.06 8.95
B2 1450+28 11.909 10.0 .. .. 4.5 24.88 1.0 .. .. .. .. 2.35 9.38
B2 1455+28 11.852 10.0 .. .. 5.2 25.61 2.0 3 S 35.48 .. 0.25 ..
B2 1457+29 11.579 5.0 6.700 6.0E6 g 3.1 25.28 1.0 .. .. .. + 1.1 ± .6 1.25 ..
B2 1502+26 11.690 13.0 .. .. 327.0d 25.69 1.0 3 S 3.98 + 0.0 ± .3 1.51 9.36
B2 1511+26 11.072 5.0 .. .. 37.8c 25.71 1.0 3 .. .. .. 0.93 ..
B2 1512+30 11.988 10.0 .. .. 2.8 24.18 .. 0 - <0.11 + 0.1 ± .4 1.89 9.01
B2 1521+28 11.838 10.0 .. .. 3.5 24.93 1.0 1 L: 2.24 + 0.2 ± .4 1.89 8.98
B2 1553+24 11.625 10.0 .. .. 2.4 23.90 1.0 1 L: 0.77 −0.06 ± .21 2.03 8.66
B2 1557+26 11.480 10.0 .. .. 7.0 23.14 1.0 1 A 0.61 + 0.06 ± .16 1.79 8.91
B2 1609+31 11.606 10.0 .. .. 4.5 24.50 1.5 0 - <0.06 −0.2 ± .5 1.88 ..
B2 1610+29 11.745 10.0 .. .. 6.2 23.35 1.0 .. .. .. −0.01 ± .18 2.04 9.04e
B2 1613+27 11.320 5.0 5.900 1.3E5 g 14.7 24.37 1.0 1 L: 0.58 + 0.0 ± .3 1.77 8.51
B2 1615+32 11.330 5.0 6.850 0.40 p 15.3 26.18 2.0 4 S1 27.14 + 3.42 ± .09 0.84 ..
11.800 13.0 9.400 1.0E8 g 66.2
B2 1615+35 11.586 10.0 .. .. 11.7 24.62 1.0 1 C 1.03 + 0.57 ± .15 1.79 ..
B2 1621+38 11.900 13.0 9.600 5.7E8 g 39.5 23.97 1.0 .. .. .. + 0.70 ± .08 2.00 8.85e
B2 1626+39 11.750 13.0 9.350 2.9E8 g 268.0c 24.81 1.0 2 L: .. + 1.93 ± .03 1.93 8.89e
B2 1637+29 12.050 13.0 8.920 2.9E8 g 5.7 24.75 1.0 0 .. .. + 1.0 ± .3 1.81 ..
B2 1638+32 11.750 5.0 .. .. 2.3 25.19 1.0 1 L: 2.55 .. 1.70 ..
B2 1643+27 12.001 13.0 .. .. 8.4 24.41 1.5 1 L: 0.94 .. 2.03 ..
B2 1652+39 11.850 13.0 7.050 2.0 p 90.8c 24.55 3.0 .. .. .. +4.05 ± .01 1.26 ..
11.850 13.0 7.900 6.0E6 g 97.9
B2 1657+32 11.661 13.0 .. .. 3.5 23.99 1.0 2 L 2.40 + 0.34 ± .08 1.73 ..
B2 1658+32 11.700 10.0 8.500 2.9E8 g 14.5 24.24 1.0 1 L: 0.96 + 0.57 ± .16 1.50 ..
B2 1658+30A 11.330 13.0 9.000 2.9E8 g 52.7c 24.20 1.5 2 L .. + 2.22 ± .06 1.86 8.94
B2 1726+31 11.786 5.0 .. .. 3.9 26.29 2.0 .. .. .. + 0.3 ± .6 1.16 8.82
3C 192 11.410 10.0 5.550 0.50 p 3.1 25.59 2.0 3 S 15.32 + 1.3 ± .3 1.32 8.07e
11.500 13.0 9.000 2.9E8 g 2.0
3C 219 11.975 13.0 6.400 0.60 p 6.2 26.86 2.0 3 S 54.94 + 1.7 ± .3 0.93 ..
12.000 13.0 8.700 5.7E7 g 9.9
3C 223 11.270 5.0 6.240 0.50 p 7.8 26.25 2.0 3 S 60.34 + 2.69 ± .27 0.02 8.15e
11.250 5.0 9.500 2.9E8 g 7.4
3C 234 11.900 13.0 7.200 2.00 p 80.0c 26.81 2.0 3 S 235.86 + 4.18 ± .07 0.20 ..
11.900 13.0 8.100 1.3E5 g 1060
3C 264 11.620 13.0 8.650 2.9E8 g 7.4 24.73 1.0 1 H: 1.21 + 1.03 ± .07 1.68 8.67e
3C 272.1 10.900 13.0 9.500 1.0E9 g 294.0c 23.54 1.0 .. .. .. + 0.79 ± .03 1.94 8.75e
3C 274 11.000 13.0 6.200 1.3E5 g 1380.0c 25.08 1.0 2 L .. + 2.16 ± .01 1.84 9.04e
3C 285 11.550 13.0 8.520 5.7E7 g 4.7 25.53 2.0 3 S: 6.59 + 2.64 ± .10 0.47 7.97e
3C 296 11.900 13.0 10.000 1.0E9 g 47.6c 24.73 1.0 1 L: 0.91 + 0.37 ± .07 1.90 8.75e
3C 303 11.400 5.0 6.800 1.30 p 3.9 26.14 2.0 4 S1 50.24 + 3.35 ± .09 0.76 ..
11.700 13.0 9.200 5.7E7 g 11.9
3C 305 11.400 5.0 10.000 5.7E8 g 17.1 25.05 1.5 3 S 17.88 + 1.38 ± .10 0.93 8.08e
3C 321 11.500 5.0 10.100 2.9E8 g 10.3 25.88 2.0 2 .. .. + 2.81 ± .08 0.07 ..
3C 326 11.320 5.0 6.400 1.3E5 g 23.7 26.37 2.0 2 C 18.60 + 0.97 ± .23 .. ..
3C 346 11.800 5.0 6.300 0.30 p 4.5 26.37 3.0 3 S .. + 1.7 ± .5 0.97 ..
11.800 5.0 8.700 5.7E7 g 7.6

Notes.

(a)

If the second component is a (young) galaxy model, then C1 = log (M/M⊙); if it is a power law, then .

(b)

For a second galaxy component, C2 is the age (in years); for a power law, C2 is the spectral index α (λ− α).

(c)

J, H, K systematically higher than the other bands, in many cases resulting in high χ2 values.

(d)

J, H, K systematically lower than the other bands, resulting in high χ2 value.

(e)

Hyperleda.

(f)

Mezcua et al. (2011).

(g)

Snellen et al. (2003).

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