\begin{table}%T2
%\centering
\par
\caption{Positions and magnitudes. For
each  star,  the first line lists  the  original  magnitudes while the
second one gives dereddened  magnitudes  adopting the reddening
law by Dean  et~al. (\cite{Dean78})  and  Rieke \&  Lebofsky (\cite{Rieke85}). }
\label{t2}
\begin{tabular}{ccccccccccc}
\hline\hline
{\rm Star} & $\alpha_{2000}$ & $\delta_{2000}$ & $E(B-V)$ & $V$ & $I$ & $J$ & $H$ & $K_{\rm s}$ &   $K_{\rm TCS}$ &   $K_{J}$  \\
&& & & $V_0$ & $I_0$ & $J_0$ & $H_0$ & $K_{\rm s0}$ & $K_{\rm TCS0}$ &   $K_{J0}$  \\
\hline
HP1-2 & 17:31:05.852M & --29:58:35.5 &  1.12  & 16.982 & 14.332 & 12.21 & 11.268 & 10.969 &  10.978 & 10.997  \\
      &               &             &       & 13.510 &  12.350  & 11.224 &  10.652 & 10.570    \\
HP1-3 & 17:31:05.872M & --29:59:18.1 &      & 17.003 & 14.358 & 12.167 & 11.146 & 10.828 & 10.838  & 10.854 \\
      &               &             &      & 13.531 & 12.376 &  11.181  & 10.530  &  10.429    \\
\hline 
\end{tabular}
\end{table}