\begin{table}%t1
\caption{\label{Table:sample}The galaxy sample.}
\small%\centering
\par
\begin{tabular}{lccccccc} 
\hline\hline\noalign{\smallskip} 
Galaxy                   & RA       & Dec       & $m_{\rm B}$         & $D$    & $M_{\rm B}$ & $A_{\rm B}$  \\
                         &  (J2000)   & (J2000)    &	            & (Mpc)  & (mag)    &  (mag)   \\
\hline
\object{Mrk 407}         & 09 47 47.6 & +39 05 04  & $15.39\pm0.49$  & 27.2   & $-16.78$ & 0.069   \\
\object{Mrk 32}          & 10 27 02.0 & +56 16 14  & $16.08\pm0.11$  & 16.4   & $-14.99$ & 0.030   \\
\object{Mrk 750}         & 11 50 02.7 & +15 01 24  & $15.76\pm0.54$  & 05.2   & $-12.82$ & 0.175   \\
\object{Mrk 206}         & 12 24 17.0 & +67 26 24  & $15.40\pm0.07$  & 24.3   & $-16.53$ & 0.071   \\
\object{Tololo 1434+032} & 14 37 08.9 & +03 02 50  & $16.91\pm0.86$  & 29.2   & $-15.42$ & 0.149   \\
\object{Mrk 475}         & 14 39 05.4 & +36 48 22  & $16.41\pm0.31$  & 11.9   & $-13.97$ & 0.052   \\
\object{I Zw 123}        & 15 37 04.2 & +55 15 48  & $15.44\pm0.08$  & 15.4   & $-15.50$ & 0.062   \\
\object{I Zw 159}        & 16 35 21.0 & +52 12 53  & $15.65\pm0.28$  & 43.8   & $-17.56$ & 0.125   \\
\hline
\end{tabular}
\tablefoot{RA, Dec, $D$ and  $A_{\rm B}$ taken from the NED 
(\protect\url{http://nedwww.ipac.caltech.edu/}).
Distances were computed using a Hubble constant of 73~km~s$^{-1}$~Mpc$^{-1}$ and taking into account the influence of the Virgo Cluster, 
the Great Attractor and the Shapley supercluster. $m_{\rm B}$ taken from 
HyperLeda (\protect\url{http://leda.univ-lyon1.fr/}; \citealp{Paturel2003}) and $M_{\rm B}$  
computed from the tabulated values of $m_{\rm B}$ and $D$. }
\end{table}