\begin{table}%T1
%\centering
\par
\caption{Positions and magnitudes from Momany et~al. (2003). For
each  star,  the first line lists  the  original  magnitudes while the
second gives dereddened  magnitudes and colours adopting the reddening
law by Dean  et~al. (1978)  and  Rieke \&  Lebofsky (1985).  Star  I-36
could not be measured in the  H~frame. $(V-I)_{\rm J}$ is Johnson, $(V-I)_{\rm C}$
is Cousins.}
\label{targets}
\begin{tabular}{ccccccccccccc}                                               
\hline
\hline
\noalign{\smallskip}
{\rm Star} & $\alpha_{2000}$ & $\delta_{2000}$ & $\Delta E(B-V)$ & $V$ & $I$ & $J$ & $H$ & $K_{\rm s}$ &   &   &   &  \\
&& &$E(B-V)$ & $V_0$ & $I_0$ & $J_0$ & $H_0$ & $K_{\rm s0}$ & $(V-I)_{\rm C0}$ & $(V-I)_{\rm J0}$ & $(V-K)_0$  & $(J-K)_0$  \\
\noalign{\vskip 0.2cm}
\noalign{\hrule\vskip 0.2cm}
\noalign{\vskip 0.2cm}
I-16 & 18:04:49.5 & --30:03:03.5 & --0.039      & 16.73 & 14.94 & 13.41 & 12.57 & 12.40 &      &      &      &      \\ 
     &            &             & 0.421 & 15.42  & 14.19 & 13.12 & 12.34 & 12.25 & 1.23 & 1.58 & 3.17 & 0.87  \\
I-18 & 18:04:49.7 & --30:03:02.5 & --0.039  & 16.73 & 15.06 & 13.79 & 13.03 & 12.96 &      &      &           \\
     &            &             & 0.421 & 15.42 & 14.31 & 13.50 & 12.80 & 12.81 &  1.11 &  1.43 &  2.61 &  0.69  \\
I-24 & 18:04:50.3 & --30:03:08.9 & --0.039 & 17.19 & 15.40 & 14.12 & 13.39 & 13.22 &      &      &            \\
     &            &             & 0.421 & 15.88 & 14.65 & 13.83 & 13.16 & 13.07 &  1.23  & 1.58 &  2.81  & 0.76  \\
I-36 & 18:04:50.9 & --30:03:48.0 & --0.026  & 16.39 & 14.42 & 12.90 & --    & 11.86 &      &      &           \\
     &            &             & 0.434 & 15.04 & 13.65 & 12.59 & 99.75 & 11.71  & 1.39 &  1.79 &  3.34 &  0.89  \\
\par
I-42 & 18:04:47.7 & --30:03:46.5 & --0.046  & 16.43 & 14.33 & 12.81 & 11.90 & 11.79 &      &      &            \\ 
     &            &             & 0.414 & 15.15 & 13.60 & 12.53 & 11.68 & 11.64  & 1.55 &  1.99 &  3.50 &  0.89  \\
 \hline \end{tabular}
\end{table}