\begin{table}%t1
%\centering
\par
 \caption{Positions, photometry, and spectral types
of the observed stars.}\label{t1}
\begin{tabular}{lcccccccc}
\noalign{\smallskip}\hline\hline \noalign{\smallskip}
Object & IAU designation & $V$ & $R$ & $I_{\rm C}$ & $J$ & $H$ & $K_{\rm s}$ & sp. type \\
\noalign{\smallskip}\hline \noalign{\smallskip}
\object{Sz~100} & J160825.8-390601 & 16.53 & 14.95 & 13.09 & 11.02 & 10.36 & 9.84 & M5 \\
\object{Sz~102} & J160829.7-390311 & 16.93 & 15.60 & 15.08 & 14.41$^1$ & 13.67$^1$ & 12.51$^1$ & ?  \\
\object{Sz~106} & J160839.7-390624 &       &       &       & 12.92 & 11.82 & 10.86 & M2.5 \\
\object{Sz~108A} & J160842.7-390617 &   &       &       & 9.76$^1$ & 9.09$^1$ & 8.78$^1$ & M3 \\
\object{Sz~108B} & J160842.8-390614 &      &       &       & 12.04 & 11.32 & 10.82 & M6 \\
\object{Sz~109} & J160848.1-390418 & 17.43 & 16.03 & 13.87 & 11.40 & 10.92 & 10.55 & M6.5 \\
\object{Sz~110} & J160851.5-390317 & 14.69 & 13.77 & 12.42 & 11.22$^1$ & 10.27$^1$ & 9.83$^1$ & M4.5 \\
\object{Sz~112} & J160855.4-390233 & 16.37 & 15.05 & 13.13 & 11.05$^1$ & 10.34$^1$ & 9.85$^1$ & M6 \\
\object{Sz~113} & J160857.7-390222 & 18.16 & 16.75 & 14.85 & 12.86$^1$ & 12.08$^1$ & 11.58$^1$ & M6 \\
\object{Sz~114} & J160901.7-390511 & 15.47 & 14.23 & 12.49 & 10.42$^1$ & 9.62$^1$ & 9.18$^1$ & M5.5 \\
\noalign{\medskip}
\object{Par-Lup3-1} & J160815.9-390307 & 19.92 & 17.60 & 15.45 & 12.60$^2$ & & & M7.5 \\
\object{Par-Lup3-1/cc~1} & J160816.0-390305 &       &       & 20.5$^3$ & & & &  M5: \\
\object{Par-Lup3-2} & J160835.7-390348 & 16.76 & 15.18 & 13.21 & 11.48 & 10.97 & 10.87 & M6 \\
\object{Par-Lup3-3} & J160849.3-390538 & 17.71 & 16.43 & 14.41 & 11.43 & 10.26 & 9.63 & M4.5 \\
\object{Par-Lup3-4} & J160851.3-390529 & 21.9: & 19.78 & 18.33 & 16.42 & 15.09 & 13.82 & M5 \\
\noalign{\smallskip}\hline
\multicolumn{9}{l}{Notes:} \\
\multicolumn{9}{l}{$^1$ $JHK$ magnitudes from Hughes et~al. (\cite{hughes94}).} \\
\par
\multicolumn{9}{l}{$^2$ $J$ magnitude from the June 2001 observations.} \\
\par
\multicolumn{9}{l}{$^3$ The value given is actually the $I_{\rm c}$ magnitude from the
FORS1 image.}\\
\end{tabular}
\end{table}