\begin{table}%t2
  \caption {\label{tab2}Integrated properties of the previously unresolved targets.}

  %\centerline
 {\begin{tabular}{lcccccccc}
    \hline\hline
    &
    &
    &
    \multicolumn{1}{c}{$J${}$^{a}$} &
    \multicolumn{1}{c}{$H${}$^{a}$} &
    \multicolumn{1}{c}{$K${}$^{a}$} &
    &
    \multicolumn{1}{c}{$d$} &
    \\
    Name &
    RA &
    Dec &
    \multicolumn{1}{c}{[mag]} &
    \multicolumn{1}{c}{[mag]} &
    \multicolumn{1}{c}{[mag]} &
    SpT &
    \multicolumn{1}{c}{[pc]} &
    Ref.     \\[0.5ex]
    \hline]
  \object{WASP-2} & 20~30~54.13 & +06~25~46.37 & $10.17\pm0.03$ &  $9.75\pm0.03$ &  $9.63\pm0.02$ & K1V  & $147\pm17^{b}$ & 1, 2\\
  \object{TrES-2} & 19~07~14.04 &+ 49~18~59.07 & $10.23\pm0.02$ &  $9.92\pm0.03$ &  $9.85\pm0.02$ & G0V & $213\pm11$ & 3, 4\\
  \object{TrES-4} & 17~53~13.06 & +37~12~42.36 & $10.58\pm0.02$ & $10.35\pm0.02$ & $10.33\pm0.02$ & F8$^{c}$ & 485v31 & 4\\[0.5ex]
  \hline
  \end{tabular}}
  \smallskip
   $^{a}$ Magnitudes are from the 2 Micron All Sky Survey (2MASS) catalogue \citep{skr06}.
  $^b$ The distance of WASP-2 has been derived indirectly from $V$~band magnitudes (see Sect.~\ref{phot}).
  $^{c}$ Since there are no good values published for TrES-4, we estimate the SpT from the $J-H$~color using templates by \citet{all99}.
   References.  (1) \citet{cam07}; (2) \citet{all99}; (3) \citet{soz07}; (4) \citet{tor08}.
\end{table}