\begin{table}%t1
\caption{\label{tab1}The complete BCG sample. }
\small%\centering
\par
\begin{tabular}{ccccccccc}
\hline \hline\noalign{\smallskip}
Abell Cl.& DC & $z$   & kpc/arcsec& BCG &RA$_{J2000}$ &  Dec$_{J2000}$& {\it HPBW}& Notes\\
\hline \noalign{\smallskip} 
262&0& 0.0161&0.328 &NGC~708&  01 52 46.458&  36 09 06.494&0.003$\arcsec$,\tablefootmark{v}&  \\ 
 347&1& 0.0187&0.380& NGC~910& 02 25 26.77&   41 49 27.3&45$\arcsec$,\tablefootmark{x1}& \\    
 400&1& 0.0232&0.468& 3C75A &  02 57 41.650&  06 01 20.717&0.0065$\arcsec$,\tablefootmark{v} & \tablefootmark{**}\\
&&&&3C75B&02 57 41.563&06 01 36.873&0.006$\arcsec$,\tablefootmark{v}&\tablefootmark{**}\\   
 407&2& 0.0470&0.922&  UGC~2489 & 03 01 51.813&  35 50 19.587&0.005$\arcsec$,\tablefootmark{v}&  \\    
 426&0&0.0176&0.358&  3C84&  03 19 48.160&  41 30 42.104&0.0018$\arcsec$,\tablefootmark{!1}& \\   
 539&2& 0.0205&0.415&  UGC~3274 &  05 16 38.91&  06 25 26.3&45$\arcsec$,\tablefootmark{x1}& \\   
 569&1 &0.0196& 0.397& NGC2~329&  07 09 08.006&  48 36 55.736&0.0035$\arcsec$,\tablefootmark{v}& \\ 
 576& 2&0.0381&0.755&  CGCG261-059&  07 22 06.980&  55 52 30.566&0.004$\arcsec$,\tablefootmark{v}&  \\   
 779&1& 0.0226&0.457&  NGC~2832&  09 19 46.87 &  33 44 59.6&45$\arcsec$,\tablefootmark{x1}&  \\  
1185&2& 0.0304& 0.608 & NGC~3550 & 11 10 38.50&   28 46 04.0&5$\arcsec$,\tablefootmark{x3}&  \\  
1213&2& 0.0468&0.918 &  4C~29.41 &  11 16 34.619&29 15 17.120&0.003$\arcsec$,\tablefootmark{v}& \\   
1228&1& 0.0350&0.697 &  IC~2738&11 21 23.06 & 34 21 24.0&5$\arcsec$,\tablefootmark{x3}&\\   
1314&1& 0.0341& 0.679 &IC~708&  11 33 59.222&  49 03 43.428&0.0022$\arcsec$,\tablefootmark{v}& \tablefootmark{*} \\ 
&&&& IC~712  &11 34 49.313 & +49 04 40.54&5$\arcsec$\tablefootmark{x3}& \tablefootmark{*} \\
1367&1& 0.0215& 0.435 &  NGC~3842 &  11 44 02.161& 19 56 59.03&5$\arcsec$,\tablefootmark{x5}&\tablefootmark{*}\\ 
&&&&3C~264 &11 45 05.014&19 36 22.94&0.0035$\arcsec$,\tablefootmark{!2}&\tablefootmark{*}\\
1656&1& 0.0232& 0.468&NGC~4874&  12 59 35.796&  27 57 33.259&0.0027$\arcsec$,\tablefootmark{v}&  \\ 
2147&1& 0.0356& 0.708& UGC~10143 & 16 02 17.027 &  15 58 28.30&5$\arcsec$,\tablefootmark{x3}& \\  
2151&1& 0.0371&0.737& NGC~6041  &  16 04 35.794&  17 43 17.551&0.0032$\arcsec$,\tablefootmark{v}&\tablefootmark{*}   \\ 
&&&& NGC~6047&16 05 08.897&   +17 43 54.31&5$\arcsec$,\tablefootmark{x3}&\tablefootmark{*}\\ 
2152&1& 0.0374&0.742&  UGC~10187& 16 05 27.176&    16 26 8.4&5$\arcsec$,\tablefootmark{x3}&  \\   
2162&1& 0.0320& 0.639 & NGC~6086 &  16 12 35.59 &  29 29 04.8&5$\arcsec$,\tablefootmark{x5}&  \\  
2197&1& 0.0303& 0.606 &NGC~6173 &  16 29 44.887&40 48 41.880&0.004$\arcsec$, \tablefootmark{v}&  \\  
2199&1& 0.0303&0.606 &  3C~338&  16 28 38.267&   39 33 04.15&0.0014$\arcsec$,\tablefootmark{!3}& \\  
2634&1& 0.0312& 0.624& 3C~465&  23 35 58.97& 26 45 16.18&0.0025$\arcsec$,\tablefootmark{!4}&\\  
2666&1 &0.0265&0.533 &  NGC~7768& 23 50 58.549&27 08 50.416& 0.0035$\arcsec$,\tablefootmark{v}& \\   \hline 
\end{tabular}
\tablefoot{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 \tablefoottext{v}{for the detected objects whose coordinates are taken by the VLBA maps and} \tablefoottext{!n}{for well known radiosources with public VLBI data:} \tablefoottext{!1}{from \citet{tay06},} \tablefoottext{!2}{from \citet{la97, ba97, la99},} \tablefoottext{!3}{from \citet{ge07} and} \tablefoottext{!4}{from \citet{ve95}.} We use \tablefoottext{xn}{for undetected radiosources for which coordinates are taken from:} \tablefoottext{x1}{, from NVSS}; \tablefoottext{x2}{from NED;} \tablefoottext{x3}{from FIRST;} \tablefoottext{x4}{from radio data of \citet{fe94};} \tablefoottext{x5}{from \citet{led95}.} In the notes: \tablefoottext{*}{is for binary clusters for which we give the name of BCGs of the two sub-clusters;} \tablefoottext{**}{indicates a dumbbell radiosource for which we consider the radioemission from both optical nuclei. }}
\end{table}