\begin{table}%t3
\caption{Complementary sample of  low mass galaxies.}\label{tab:Extendedgalaxyset}
    \small%\centerline
{
        \begin{tabular}{cccccc}
        \hline \hline
Galaxy &     $l$    & $b$ &    $d$ & $V_r$ &  $M$   \\
        \hline
N2403    & 149.6  &  29.3  &3.3  & 227  &11.8    \\
N4236    &  12.3  &  47.3  &3.9  & 118  &11.5    \\
Circinus & 311.3  &   3.7  &3.3  & 268  &11.5    \\
N55      & 332.6  & --75.6  &1.6  &  96  &11.5    \\
N7793    &   4.4  & --77.1  &4.1  & 230  &11.5    \\
N300     & 299.2  & --79.4  &2.1  & 101  &11.3    \\
N1569    & 143.6  &  11.2  &2.4  &  47  &11      \\
N404     & 126.9  & --27.1  &3.6  & 115  &10.8    \\
N3109    & 262.1  &  23.0  &1.3  & 194  &10.5    \\
IC5152   & 343.8  & --50.1  &1.7  &  85  &10      \\
SexA,B   & 240.3  &  42.0  &1.4  & 165  &10      \\
N6822    &  25.3  & --18.3  &0.5  &  45  &10      \\
N1311    & 264.2  & --52.6  &3.1  & 425  & 9.8    \\
IC1613   & 129.7  & --60.5  &0.7  &--155  & 9.8    \\
WLM      &  75.8  & --73.6  &0.9  & --65  & 9.7    \\
VIIZw403 & 127.8  &  37.3  &4.5  &  50  & 9.6    \\
SagDIG   &  21.0  & --16.5  &1.1  &  7   & 9.1    \\
PegDIG   &  94.7  & --43.5  &0.8  & --22  & 8.9    \\
LeoA     & 196.8  &  52.4  &0.7  & --18  & 8.8    \\
DDO210   &  34.0  & --31.3  &0.9  & --24  & 8.7    \\
DDO155   & 310.8  &  76.9  &1.5  & 183  & 8.6    \\
Phoenix  & 272.0  & --68.9  &0.4  & --34  & 7.7    \\
\hline
\end{tabular}}
\medskip
This sample is added to the sample of Table~\ref{tab:ExternalGalaxiesAdopted}. The effect of these galaxies can be considered as a perturbation. The coordinates $l$ and~$b$ are in~$^{\circ}$, the distances~$d$ are in Mpc (as in the previous table
we omit the uncertainties on the distances and velocities), the
radial velocity $V_r$ is in km~s$^{-1}$, and the galaxy masses are in solar
units. They are expressed as $\log M$.
\end{table}