Table 1:

The complete BCG sample.

Abell Cl.	DC	z	kpc/arcsec	BCG	RAJ2000	DecJ2000	HPBW	Notes
262	0	0.0161	0.328	NGC 708	01 52 46.458	36 09 06.494	0.003 ,v
347	1	0.0187	0.380	NGC 910	02 25 26.77	41 49 27.3	45 ,x1
400	1	0.0232	0.468	3C75A	02 57 41.650	06 01 20.717	0.0065 ,v	**
				3C75B	02 57 41.563	06 01 36.873	0.006 ,v	**
407	2	0.0470	0.922	UGC 2489	03 01 51.813	35 50 19.587	0.005 ,v
426	0	0.0176	0.358	3C84	03 19 48.160	41 30 42.104	0.0018 ,!1
539	2	0.0205	0.415	UGC 3274	05 16 38.91	06 25 26.3	45 ,x1
569	1	0.0196	0.397	NGC2 329	07 09 08.006	48 36 55.736	0.0035 ,v
576	2	0.0381	0.755	CGCG261-059	07 22 06.980	55 52 30.566	0.004 ,v
779	1	0.0226	0.457	NGC 2832	09 19 46.87	33 44 59.6	45 ,x1
1185	2	0.0304	0.608	NGC 3550	11 10 38.50	28 46 04.0	5 ,x3
1213	2	0.0468	0.918	4C 29.41	11 16 34.619	29 15 17.120	0.003 ,v
1228	1	0.0350	0.697	IC 2738	11 21 23.06	34 21 24.0	5 ,x3
1314	1	0.0341	0.679	IC 708	11 33 59.222	49 03 43.428	0.0022 ,v	*
				IC 712	11 34 49.313	+49 04 40.54	5 x3	*
1367	1	0.0215	0.435	NGC 3842	11 44 02.161	19 56 59.03	5 ,x5	*
				3C 264	11 45 05.014	19 36 22.94	0.0035 ,!2	*
1656	1	0.0232	0.468	NGC 4874	12 59 35.796	27 57 33.259	0.0027 ,v
2147	1	0.0356	0.708	UGC 10143	16 02 17.027	15 58 28.30	5 ,x3
2151	1	0.0371	0.737	NGC 6041	16 04 35.794	17 43 17.551	0.0032 ,v	*
				NGC 6047	16 05 08.897	+17 43 54.31	5 ,x3	*
2152	1	0.0374	0.742	UGC 10187	16 05 27.176	16 26 8.4	5 ,x3
2162	1	0.0320	0.639	NGC 6086	16 12 35.59	29 29 04.8	5 ,x5
2197	1	0.0303	0.606	NGC 6173	16 29 44.887	40 48 41.880	0.004 , v
2199	1	0.0303	0.606	3C 338	16 28 38.267	39 33 04.15	0.0014 ,!3
2634	1	0.0312	0.624	3C 465	23 35 58.97	26 45 16.18	0.0025 ,!4
2666	1	0.0265	0.533	NGC 7768	23 50 58.549	27 08 50.416	0.0035 ,v

Notes. In Col. 1 we report the name of the Abell cluster, in Col. 2 the distance class (DC), in Col. 3 the redshift z of the cluster, in Col. 4 we report the kpc/arcsec conversion for each cluster, in Col. 5 the name of the BCG, in Cols. 6 and 7 we give the RA and Dec in J2000 coordinates of the BCG. In Col. 8 we give the angular resolution of maps used to estimate the core coordinates. We use ^(v) for the detected objects whose coordinates are taken by the VLBA maps and ^(!n) for well known radiosources with public VLBI data: ^(!1) from Taylor et al. (2006a), ^(!2) from Lara et al. (1999,1997); Baum et al. (1997), ^(!3) from Gentile et al. (2007) and ^(!4) from Venturi et al. (1995). We use ^(xn) for undetected radiosources for which coordinates are taken from: ^(x1) , from NVSS ^(x2) from NED; ^(x3) from FIRST; ^(x4) from radio data of Feretti & Giovannini (1994); ^(x5) from Ledlow & Owen (1995). In the notes: ^(*) is for binary clusters for which we give the name of BCGs of the two sub-clusters; ^(**) indicates a dumbbell radiosource for which we consider the radioemission from both optical nuclei.