\begin{table}%T2
      \caption{Observational information.}
      \label{LogObsTable}
 %\centerline
{
      \begin{tabular}{lllllll}
         \hline\hline
         \noalign{\smallskip}
         OBJECT       & Filter /                 & Standard  & Average                & \texpo & Number  & Notes$^{{e}}$ \\ 
                      & Telescope$^{{a}}$ &   star    & counts$^{{b}}$  &        & frames  & \\ 
         \noalign{\smallskip}
         \hline
         \noalign{\smallskip}
         \glftn       & $K$ / C &  SAO~12585 / SAO~23728   & 120    & 0.20 & 1536 & N! \\ 
         \glftss      & $K$ / U &  CMC~302423 / CMC~601567 &  21    & 0.13 & 1200 & N \\ 
         \glf         & $J$ / U &  CMC~401688 / CMC~302688 &  31    & 0.20 & 1500 & -- \\ 
                      & $H$ / U &  SAO~24017 / SAO~23967   & 116    & 0.05 & 4000 & N! \\ 
                      & $K$ / U &  SAO~24017               & 474    & 0.02 & 3500 & U \\ 
                      & \brq / U & SAO~24017             & 107    & 0.13 & 2000 & U \\ 
                      & Con / U &  SAO~24017             &  70    & 0.13 & 2000 & U \\ 
                      & $H$ / C &  SAO~23999$^{c}$ / SAO~24017 & 120  & 0.06 & 1280 & N \\ 
                      & $K$ / C &  SAO~24098 / SAO~24017   & 537    & 0.06 & 1000 & U \\ 
         \lkhao\      & $J$ / U &  SAO~57254 / SAO~57264   &  73    & 0.05 & 3000 & C \\ 
                      & $H$ / C &  SAO~57239 / SAO~57264   & 692    & 0.06 & 1536 & C \\ 
         \sfour       & $H$ / U &  SAO~58357 / SAO~58383   &  65    & 0.13 & 3000 & U \\ 
                      & $K$ / C &  SAO~58343 / SAO~58272   &  54    & 0.06 & 1536 & U \\ 
         \sone\       & $H$ / UC&  SAO~58357               &  56    & 0.20 & 2000 & N \\ 
                      & $K$ / U &  SAO~58343               & 119    & 0.05 & 2000 & N \\ 
                      & $K$ / C &  SAO~58343 / SAO~58272   & 122    & 0.20 & 1536 & N \\ 
         \sttft       & $K$ / C &  SAO~58343 / SAO~58272   & 190    & 0.06 & 1536 & U \\ 
                      & $H$ / C &  SAO~58357               & 107    & 0.10 & 1536 & U \\ 
         \ngctwo      & $K^{d}$ / C &  SAO~132480 & 853    & 0.06 & 1536 & U \\ 
                      & $H$ / C &  SAO~132410 / SAO~132434 & 144    & 0.06 & 1536 & U \\ 
         \mont        & $K$ / U &  SAO~132881 / SAO~132874 &  15    & 0.20 & 1536 & U \\ 
         \mon         & $K$ / C &  SAO~133884 / SAO~132874$^{c}$ & 106 & 0.06 & 1536 & N \\ 
                      & $H$ / U &  SAO~132874              & 139    & 0.20 & 2000 & N \\ 
                      & $K$ / U &  SAO~132884              &  75    & 0.02 & 2000 & N \\ 
         \gfive       & $K$ / C &  SAO~78056$^{{c}}$ / SAO~77997& 23  & 0.3 & 768  & U \\ 
         \stwo/3      & $K$ / C &  SAO~95350               &  41    & 0.20 & 1536 & N \\ 
         \gla -E/W    & $H$ / U &  SAO~114047 / SAO~114O94 & 209    & 0.25 & 1000 & N!/C \\
                      & $K$ / C &  SAO~114047 / SAO~114O80 &  62    & 0.06 & 1792 & U \\
         \fan         & $K$ / U &  SAO~114047 / SAO~114O94 &  88    & 0.13 & 2000 & U \\
         \glb         & $H$ / U &  SAO~95987               & 140    & 0.05 & 3000 & U \\ 
                      & $H$ / C &  SAO~95987               & 120    & 0.06 & 2048 & N! \\ 
                      & $K$ / C &  SAO~114234 / SAO~114245 &  68    & 0.06 & 1792 & U \\ 
         \sir         & $K$ / C &  SAO~76077 / SAO~70120   & 330    & 0.06 & 2048 & U \\ 
                      & $H$ / C &  SAO~70120 / SAO~70129   & 109    & 0.13 & 1280 & U \\ 
         \glt         & $H$ / U &  SAO~70099 / SAO~49777   &  29    & 0.13 & 2000 & -- \\ 
                      & $K$ / U &  SAO~70052               & 381    & 0.05 & 1500 & N! \\
                      & $K$ / C &  SAO~70052 / SAO~49730   & 274    & 0.06 & 2048 & N! \\
%         \ws          & $K$ / U &  SAO~49899 / SAO~49946   &  12    & 0.25 & 600  & -- \\ 
         \sonef       & $K$ / C &  SAO~20051 / SAO~19948   & 250    & 0.06 & 1600 & N \\ 
         \ngcsfte     & $K$ / C &  SAO~20455 / SAO~20563   &  21    & 0.20 & 1536 & N! \\
         \hline
      \end{tabular}}
\par
         \medskip
      $^{{a}}$ U: UKIRT. C: 3.5~m telescope at Calar Alto.\\
      $^{{b}}$ Average peak counts per frame.\\
      $^{{c}}$ These stars were found to be close binaries and so not included in the reduction.\\
      $^{{d}}$ Object was too bright at $K$ and so a narrow-band filter at 2.26~$\mu$m was used instead.\\
      $^{{e}}$ Main features observed in the reconstructed images. N:
	Bright nebula likely to be associated to the outflow cavity. N!:
	Very low level or hardly resolved nebulosity. C: Close companion
	(with a separation $<$1\farcs5). U: Unresolved source. --:
	Reconstruction not possible due to the low number of
	photons per individual frame.
\end{table}