\begin{table}%t1
%\centering
\par
\caption{Dwarf galaxies
  within the vicinity of the MW. The first column is a running number
  used throughout this text; the parentheses contain the running
  number used in Sect.~\ref{sec:prob} after excluding the SMC and UMi.
  $D$ and $eD$ are the distance and its uncertainty, respectively.
  $l$, $b$ are the Galactic longitude and latitude, respectively, as
  seen from the Sun and defined such that $l=0, b=0$ points towards
  the Galactic centre which is assumed to lie at a distance
  $D_\odot=8.5$~kpc from the Sun, and $l$ increases in anticlockwise
  direction.  The Galactocentric distance of the dwarf is given by~$R$.  
  The name of the dwarf is given in the 7th column.  The data
  are from Mateo (\cite{mateo98}, Table~2), except that for the LMC
  $D$ and $eD$ are taken from Salaris et~al. (\cite{salaris03}) and
  Clementini et~al. (\cite{clementini03}), and likewise for the SMC
  from Dolphin et~al. (\cite{dolphin01}).  The remaining columns
  contain the plane-fitting results for the innermost $N$ dwarves
  (Sect.~\ref{sec:plane}): $R_{\rm cut}$ is the largest distance to the
  Galactic centre of this sample, and the fitted plane has a root-mean
  square height $\Delta$ and a distance to the Galactic centre $D_{\rm
    P}$. For comparison, the final column lists the root-mean-square
  height $\Delta_2(R_{\rm cut})$ for samples of $4\times10^5$
  theoretical dwarves with an isotropic isothermal radial number
  density profile ($p=2$) and radial cutoff~$R_{\rm cut}$.
        \label{tab:MWsat}}
    \begin{tabular}[h!]{ccccccccccccc} \hline\hline
\par
      satellite &$D$     &$eD$    &$l$     &$b$   &$R$ 
     &Name &$R_{\rm cut}$ &$\Delta$ &$\Delta/R_{\rm cut}$
       &$D_{\rm P}$ &&$\Delta_2$ \\
\par
      number    &[kpc]   &[kpc]   &[deg]   &[deg] &[kpc] 
     & & [kpc] &[kpc]    & &[kpc]     & &[kpc]\\
\par
           \hline
\par
      1(1)     &  24     &   2      &   5.6  & $-14.1$ &  16  
     & Sgr &-- &-- &-- &-- &&--\\
      2(2)     &  50.8   &   2.2    & 280.5  & $-32.9$ &  50  
     & LMC &-- &-- &-- &-- &&--\\
      3(--)     &  59.7   &   2.2    & 302.8  & $-44.3$ &  57  
     & SMC &-- &-- &-- &-- &&--\\
      4(--)     &  66     &   3      & 105.0  & $+44.8$ &  68  
     & UMi &  68 &   2.5 &0.04 & 0.6 &&  23 \\
      5(3)     &  79     &   4      & 287.5  & $-83.2$ &  79  
     & Sculptor&  79 &  11.8 &0.15 & 3.0 &&  27\\
      6(4)     &  82     &   6      &  86.4  & $+34.7$ &  82  
     & Draco   &  82 &  11.0 &0.13 & 3.2 &&  28\\
      7(5)     &  86     &   4      & 243.5  & $+42.3$ &  89  
     & Sextans &  89 &  13.5 &0.15 & 1.2 &&  30\\
      8(6)     & 101     &   5      & 260.1  & $-22.2$ & 103  
     & Carina  & 103 &  14.2 &0.14 & 1.4 &&  34\\
      9(7)     & 138     &   8      & 237.1  & $-65.7$ & 140  
     & Fornax  & 140 &  23.9 &0.17 & 2.0 &&  47\\
     10(8)     & 205     &  12      & 220.2  & $+67.2$ & 208  
     & LeoII   & 208 &  23.2 &0.11 & 1.9 &&  69\\
     11(9)     & 250     &  30      & 226.0  & $+49.1$ & 254  
     & LeoI    & 254 &  26.4 &0.10 & 1.9 &&  85\\
     12(10)    & 445     &  30      & 272.2  & $-68.9$ & 445  
     & Phoenix & 445 &  32.0 &0.07 & 2.1 && 148\\
     13(11)    & 490     &  40      &  25.3  & $-18.4$ & 483  
     & NGC 6822& 483 &  86.4 &0.18 & 3.5 && 161\\
     14(12)    & 690     & 100      & 196.9  & $+52.4$ & 695  
     & Leo A   & 695 & 100   &0.14 & 3.5 && 232\\
     15(13)    & 880     &  40      & 322.9  & $-47.4$ & 875  
     & Tucana  & 875 & 123   &0.14 & 3.5 && 292\\
     16(14)    & 955     &  50      &  94.8  & $-43.5$ & 956  
     & Pegasus & 956 & 159   &0.17 & 3.3 && 319\\
\hline
    \end{tabular}
\end{table}