\begin{table}%t3
\renewcommand{\arraycolsep}{1.2}
\caption {Absolute extinction corrected magnitudes, 
ages, velocity dispersion~$\sigma$, projected half-light radius 
$r_{\rm hp}$.    $M_{\rm dyn}$ with 1$\sigma$-uncertainties $\Delta M$, photometric mass  $M_{\rm ph}$.  \label{massestable}}
%\centerline
 {
\begin{tabular}{lcccccccccc}
\hline
\hline
Cluster      &  $M_K$(0)$^a$   & $A_V$  & Age         & $\sigma$     & $r_{\rm hp}$     &   $M_{\rm dyn}$  &  $L_K/M$ & $M_{\rm ph}$ & $M_{\rm dyn}$/$M_{\rm ph}$ &  $P/G$ \\
             &  mag        & mag    & [10$^6$~yr]  & [km~s$^{-1}$]       & [pc]         & [10$^6$~$M_{\odot}$]  & [$L_{\odot}$/$M_{\odot}$]  & [10$^6$~$M_{\odot}$] & & 10$^9~M_{\odot}^2$/pc$^4$]  \\\hline
$[$W99$]$2   & --17.4~$\pm$~0.1   &  $\approx$0  & 6.6~$\pm$~0.3 & 14.1~$\pm$~1.0$^b$  & 8.0~$\pm$~1.5 & $\rm 3.0^{+1.2}_{-1.0}$    & $\rm 64^{+40}_{-23}$   & $\rm 2.7^{+0.8}_{-0.5}$   & $\rm 1.0^{+0.8}_{-0.4}$  & $\rm 1.9^{+2.7}_{-1.2}$  \\
$[$W99$]$15  & --15.5~$\pm$~0.1   &  1           & 8.7~$\pm$~0.3 & 20.2~$\pm$~1.5 & 1.4~$\pm$~0.2 & $\rm 1.0^{+0.3}_{-0.15}$   & $\rm 34^{+10}_{-10}$   & $\rm 0.5^{+0.1}_{-0.1}$   & $\rm 1.9^{+1.2}_{-0.5}$ & $\rm 60^{+50}_{-36}$  \\
S1\_1        & --15.7~$\pm$~0.1   &  4.6         & 8.0~$\pm$~0.3 & 12.5~$\pm$~3   & 3.6~$\pm$~0.3 & $\rm 1.0^{+0.6}_{-0.4}$    & $\rm 38^{+28}_{-16}$   & $\rm 0.7^{+0.2}_{-0.1}$   & $\rm 1.5^{+1.4}_{-0.8}$ & $\rm 2.9^{+1.5}_{-1.4}$  \\
S1\_2        & --15.4~$\pm$~0.2   &  2           & 8.3~$\pm$~0.3 & 11.5~$\pm$~2.0 & 3.6~$\pm$~0.4 & $\rm 0.8^{+0.4}_{-0.3}$    & $\rm 37^{+33}_{-14}$   & $\rm 0.5^{+0.3}_{-0.1}$   & $\rm 1.7^{+1.4}_{-1.0}$ & $\rm 1.4^{+1.1}_{-0.9}$  \\
S1\_5        & --14.8~$\pm$~0.1   &  2           & 8.5~$\pm$~0.3 & 12.0~$\pm$~3   & 0.9~$\pm$~0.6 & $\rm 0.4^{+0.6}_{-0.3}$    & $\rm 46^{+50}_{-21}$   & $\rm 0.3^{+0.04}_{-0.05}$   & $\rm 1.4^{+1.9}_{-1.0}$ & $\rm 103^{+767}_{-94}$  \\
2000\_1      & --16.8~$\pm$~0.3   &  $\approx$10 & 8.5~$\pm$~0.3 & 20.0~$\pm$~3   & 3.6~$\pm$~1.0 & $\rm 2.4^{+1.3}_{-0.9}$    & $\rm 46^{+226}_{-30}$  & $\rm 1.7^{+0.9}_{-0.6}$   & $\rm 1.5^{+3.2}_{-1.2}$ & $\rm 16^{+44}_{-14}$  \\
S2\_1        & --15.2~$\pm$~0.2   &  1.2         & 9.0~$\pm$~0.3 & 11.5~$\pm$~2.0 & 3.7~$\pm$~0.5 & $\rm 0.9^{+0.5}_{-0.4}$    & $\rm 27^{+29}_{-13}$   & $\rm 0.3^{+0.12}_{-0.06}$   & $\rm 2.7^{+2.5}_{-1.5}$ & $\rm 0.6^{+0.6}_{-0.3}$  \\
S2\_2        & --15.3~$\pm$~0.1   &  0.5         & 9.0~$\pm$~0.3 &  9.5~$\pm$~2.0 & 2.5~$\pm$~0.5 & $\rm 0.4^{+0.26}_{-0.17}$  & $\rm 72^{+72}_{-33}$   & $\rm 0.4^{+0.08}_{-0.03}$   & $\rm 1.0^{+0.9}_{-0.6}$ & $\rm 3.5^{+6.0}_{-2.1}$  \\
S2\_3        & --14.8~$\pm$~0.1   &  $\approx$0  & 9.0~$\pm$~0.3 &  7.0~$\pm$~2.0 & 3.0~$\pm$~1.0 & $\rm 0.25^{+0.32}_{-0.17}$ & $\rm 70^{+168}_{-42}$   & $\rm 0.24^{+0.07}_{-0.03}$   & $\rm 1.0^{+1.7}_{-0.8}$ & $\rm 0.7^{+3.3}_{-0.5}$  \\
NGC 1487-1   & --14.2~$\pm$~0.1   &  0.6         & 8.4~$\pm$~0.5 & 13.7~$\pm$~2.0$^c$ & 2.3~$\pm$~0.5 & $\rm 1.2^{+0.7}_{-0.5}$    & $\rm 8.1^{+6.5}_{-3.3}$ & $\rm 0.15^{+0.05}_{-0.02}$  & $\rm 8.2^{+6.3}_{-4.5}$ & $\rm 0.80^{+1.7}_{-0.5}$  \\
NGC 1487-2   & --14.2~$\pm$~0.1   &  1.0         & 8.5~$\pm$~0.5 & 11.1~$\pm$~1.8 & 1.0~$\pm$~0.3 & $\rm 0.2^{+0.11}_{-0.08}$  & $\rm 48^{+36}_{-19}$   & $\rm 0.16^{+0.05}_{-0.02}$  & $\rm 1.3^{+1.0}_{-0.7}$ & $\rm 26^{+46}_{-16}$  \\
NGC 1487-3   & --13.4~$\pm$~0.3   &  0.5         & 8.5~$\pm$~0.5 & 14.3~$\pm$~1.0 & 1.8~$\pm$~0.3 & $\rm 0.6^{+0.20}_{-0.13}$  & $\rm 7.7^{+5.2}_{-3.3}$  & $\rm 0.076^{+0.04}_{-0.03}$ & $\rm 8.2^{+9.6}_{-4}$ & $\rm 0.6^{+0.3}_{-0.4}$  \\\hline
\end{tabular}}
\smallskip
\par
$^a$ {Distance moduli of 31.41 and 30.13 for NGC 4038/4039 and NGC 1487, respectively;}
$^b$ {average value from ISAAC,14.0~$\pm~0.8$ and UVES, 14.3~$\pm$~0.5;}
$^c$ {average value from ISAAC, $13.4\pm1.5$ and UVES, 
$15.4\pm2.0$.}
\par
\end{table}