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Table 3:

Parameters for BCGs.

BCG 		pc j/cj $\beta \cos \theta$ $S_{\rm c,5}$ Log  $P_{\rm c,5}$ $S_{\rm t,408}$ Log  $P_{\rm t,408}$ $S_{\rm VLBI}$/ Core Notes
  structure ratio   mJy W/Hz mJy W/Hz $S_{\rm c, 5~GHz}$($\%$) dominance  
NGC 708 c - - 5 21.47 364 23.33 60 0.26 5
NGC 910 n.d. - 2 - - - - <25 - 5
3C 75A 1s $\geq$6.2 $\geq$0.35 6 21.87 190 23.37 100 0.60 1
3C 75B 1s $\geq4.6$ $\geq$0.3 20 22.39 190 23.37 100 2 1
3C 84 2s 2 0.14 28.17 $\times $ 103 25.29 51.68 $\times $ 103 25.56 80 70.79 2
UGC 3274 n.d. - - <1.4 - - - - - 5
UGC 2489 1s $\geq$2.8 $\geq$0.2 4 22.32 2.83 $\times $ 103 25.17 90 0.13 3
NGC 2329 1s $\geq$4.5 $\geq$0.29 160 23.14 1300 24.05 50 4.3 4
CGCG 261-059 1s $\geq$1.8 $\geq$0.12 1.5 21.71 6.54 22.34 100 1.8 5
NGC 2832 n.d. - - 2.4 - - - <21 - 5
NGC 3550 n.d. - - <1.4 - - - - - 5
4C 29.41 1s $\geq$3.8 $\geq$0.26 41 23.33 135.2 23.84 100 8.71 6
IC 2738 n.d. - - - - - - - - 5
IC 708 1s $\geq$6.5 $\geq$0.36 110 23.47 901.1 24.39 40 5.62 7
IC 712 n.d. - - 14.02 22.58 48.72 23.12 <3 4.37 11
NGC 3842 n.d. - - 9 22.98 101.88 23.03 <8 0.36 11
3C 264 1s $\geq$6 $\geq$0.34 200 23.32 17 $\times $ 103 25.25 100 1.17 8
NGC 4874 1s $\geq$1.6 $\geq$0.09 1.1 21.13 351.96 23.63 100 0.08 9
UGC 10143 n.d. - - <2 <21.77 14.87 22.64 - <1.35 5
NGC 6041A c - - $\leq$0.9 $\leq$21.92 21.5 22.84 100 1.45 5
NGC 6047 n.d. - - 8.3 22.42 1960 24.80 <7 0.28 12
UGC 10187 n.d. - - <2 <21.81 111.7 23.56 - <0.41 5
NGC 6086 n.d. - - <1 <21.37 201.35 23.68 - <0.12 5
NGC 6173 1s $\geq$1.4 $\geq$0.07 3.7 21.89 12.97 22.44 40 2.40 5
3C 338 2s 2.2 0.16 480 24.01 18.12 $\times $ 103 25.59 30 3.47 10
3C 465 1s $\geq$20 $\geq$0.54 246 23.74 10.38 $\times $ 103 25.37 100 2.57 8
NGC 7768 1s $\geq$1.1 $\geq$0.02 0.74 21.08 2.6 21.62 100 1.17 5

B2 0836+29II 		1s $\geq$20 $\geq$0.54 131 24.31 1139 25.24 100 11.20 13
Hydra A 2s 1.2 0.04 168 24.08 132 $\times $ 103 26.98 100 0.58 14
4C 26.42 2s 1.4 0.07 53 23.71 3153 25.48 80 2.04 15
3C 317 2s 1.5 0.08 310 23.93 132 $\times $ 103 26.56 100 0.72 16
B2151+174 2s 4 0.27 164 25.40 538 25.92 100 53 17
PKS 2322-123 2s 1.2 0.04 59.3 24.0 7.2 $\times $ 103 26.11 80 1.66 18
PKS 1246-410 1s $\geq$9 0.34 64.4 22.27 2463 23.86 30 0.76 19

Notes.  $S_{\rm t,408}$: 1) From NVSS with $\alpha\sim0.5$, 2) from Parma et al. (1991) with $\alpha\sim0.5$; 3) from Pedlar et al. (1990) where $\alpha\sim0.5$, 4) from Bondi et al. (1993), 5) from Feretti & Giovannini (1985), 6) from Owen & Ledlow (1997) with $\alpha\sim0.5$, 7) from Vallee et al. (1979) where $\alpha\sim0.6$, 8) from Feretti & Giovannini (1994), 9) from Giovannini et al. (2001) and NED information with $\alpha\sim0.5$, 10) from Feretti & Giovannini (1987) with $\alpha\sim0.5$, 11) from Owen & Ledlow (1997), 12) from Taylor et al. (2002) and NED information, 13) from Venturi et al. (1995), 14) from Taylor (1996); Taylor et al. (1990), 15) from Liuzzo et al. (2009a), 16) from Venturi et al. (2004), 17) from Augusto et al. (2006) and from NED with $\alpha\sim0.5$ (408 MHz) and  $\alpha\sim 0$ (5 GHz), 18) from Taylor et al. (1999) and NED information and 19) from Taylor et al. (2006b) assuming $\alpha=0.5$. $S_{\rm c}$ is for the arcsecond core flux density at 5 GHz and $S_{\rm VLBI}$ is a correlated flux density at 5 GHz in our VLBI data.
We give the name of the BCG (Col. 1), the parsec-scale morphology (Col. 2: core (c), one sided (1 s) or two sided (2 s) jet structure), the jet/counterjet surface brightness ratio (Col. 3), $\beta$cos$\theta$ (Col. 4), the arcsecond core flux density $S_{\rm c,5}$ at 5 Ghz (Col. 5), the arcsecond core power Log  $P_{\rm c,5}$ at 5 GHz (Col. 6), the total arcsecond flux density $S_{\rm t,408}$ (Col. 7) and the total arcsecond power Log  $P_{\rm t,408}$ (Col. 8) at 408 MHz, the total VLBI flux density and arcsecond core flux density ratio $S_{\rm VLBI}$/ $S_{\rm c,5}$ at 5 GHz (Col. 9), the core dominance (see Sect. 5.2) (Col. 10). The last column is for the notes.


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