\begin{table}%t1
  \caption{Summary of targets and references.
  Tip-tilt star magnitude and separation to the target based on USNO-A2.0 \citep{Monet98}. 
  All distances are photometric, based on the relations of \citet{Knapp04} between the spectral type, and $M_J$, and $M_K$ (except for \SD), assuming non-binarity. }
  \label{targets}
  %\centerline
{
  \begin{tabular}{lccccccc}
    \hline
    \hline
    \noalign{\smallskip}
    NACO targets  & Tip/tilt($R$) & Sp.T. $^1$&  $J\;^2$ (mag)  &  $H\;^2$ (mag) & Dist. (pc) & $\mu_\alpha$ (mas/yr) & $\mu_\delta$ (mas/yr) \\
      \hline
    \noalign{\smallskip}
    \object{2MASSI J0756252+124456}$^3$        & $16.3, 37\arcsec$ & L6$^3$ & $16.66\pm 0.14$ & $15.76\pm 0.15$ & 38 & $-3\pm13$ & $-93\pm43$ \\ 
    \object{2MASS J09393548$-$2448279}$^4$ & $12.2, 30\arcsec$ & T8 & $15.98\pm 0.11$ & $15.80\pm 0.15$ & 9  & 490$^4$ & $-1040$$^4$ \\ 
    \object{2MASSW J1036530$-$344138}$^5$ & $17.6, 17\arcsec$& L6$^5$ &  $15.62\pm 0.05$ & $14.45\pm 0.04$ & 22  & $-123\pm20$ & $-426\pm20$ \\\ 
    \object{SDSS J204749.61$-$071818.3}$^6$ & $13.8, 12\arcsec$ & T0: & $16.47\pm 0.20$ & $15.91\pm 0.20$ & 32 & $-3\pm20$ & $-274\pm20$ \\ 
     \hline
       Lick targets                                   & Tip/tilt($R$)               & Sp.T. &           $J$ (mag)      &                      $K$s (mag)           & Distance (pc) & $\mu_\alpha$ (mas/yr) & $\mu_\delta$ (mas/yr) \\
        \hline \noalign{\smallskip}
        \object{2MASS J16262034+3925190}$^7$        & $14.5, 35\arcsec$ & dL4$^8$ & $14.44\pm 0.03$ & $14.47\pm 0.07$ & 37$^9$  & $+286^7$ & $-1237^7$\\ 
    \object{{SIMP} J013656.5+093347.3}$^{10}$           &                                  & T2.5$^{10}$ & $13.46\pm 0.03$ & $12.56\pm 0.03$ & 7.6$^{10}$  & $-4^{10}$ & $+1241^{10}$\\       
   \hline
\end{tabular}}
\medskip
\par
$^1$  Spectral types from \citet{Burga06cl} except for \Ms,  \Mt\ , 2MASS~J1626 and \IPMS. 
$^2$  Target photometry from 2MASS \citep{Skrut06}. 
$^3$ \citet{Kirkp00}.  
$^4$ \citet{Tinne05}.  
$^5$ \citet{Gizis02}. 
$^6$ \citet{Knapp04}.  
$^7$ \citet{Burga04sd}. 
$^8$ \citet{Burga07sL} 
$^9$ The distance is based on the $K$ magnitude only, as the parallax measurement of sdL7 subdwarf revealed a $M_K$ similar to the solar-metallicity L7 dwarfs, while the subdwarf is more than 1~magnitude brighter in the $J$ band \citep{Burga08sd}. 
$^{10}$  \citet{Artig06}. They report a distance of $6.4\pm 0.4$~pc.
\end{table}