\begin{table}%t3
\caption{Masses of HR~8799 b / c / d from luminosity (and absolute $K$-band
magnitude) using
various evolutionary models.}
\label{tab_masses_from_models}
%%\centering

\par
\begin{tabular}{l|ccccccccc}
\hline\hline
HR~8799 b & \multicolumn{9}{c}{Luminosity $\log{L/L_{\odot}}= -5.1~\pm~0.1$
\citep{marois-et-al-2008}} \\
\hline
Model &  \multicolumn{9}{c}{Mass [{\it M}$_{{\rm Jup}}$] at age}\\
& 20 Myr & 30 Myr & 60 Myr & 100 Myr & 160 Myr & 590 Myr & 730 Myr & 1000 Myr &
1128 Myr  \\
\hline
 \citet{burrows-et-al-1997} & 3.5--4.5 & 4.5--6 & 7--8.5 & 9--11 & 11.5--12.5 & 22--26 & 25--30 & 28--33 & 30--36\\
 \citet{marley-et-al-2007}$^a$ & 3--5 & 4--7 & 6--10 & & & & & &\\
 \citet{chabrier-et-al-2000} & & & & & & 21--26 & & 30--35 &\\
 \citet{baraffe-et-al-2003} & & 4--5 & 6--7 & 9--10 & & 21--26 & & 30--35 &\\
 \citet{baraffe-et-al-2008}$^b$ & & & $\sim$7  & $\sim$9 & & & & &\\
\hline
 \citet{baraffe-et-al-2003}$^c$ & & $\sim$5.5 & $\sim$8.5 & $\sim$10.5 & &
$\sim$30 & & $\sim$38 &\\
\hline
HR~8799 c / d & \multicolumn{9}{c}{Luminosity $\log{L/L_{\odot}}=
-4.7~\pm~0.1$ \citep{marois-et-al-2008}} \\
\hline
Model &  \multicolumn{9}{c}{Mass [{\it M}$_{{\rm Jup}}$] at age}\\
& 20 Myr & 30 Myr & 60 Myr & 100 Myr & 160 Myr & 590 Myr & 730 Myr & 1000 Myr &
1128 Myr  \\
\hline
 \citet{burrows-et-al-1997} & 6--7.5 & 7.5--9.5 & 11--12 & 12.5--13 & 13--13.5 & 30--38 & 35--43 & 40--48 & 41--50\\
 \citet{marley-et-al-2007}$^a$ & 6--8 & 8--10 & & & & & & &\\
 \citet{chabrier-et-al-2000} & & 6--7 & 8--10 & 10--11 & & 28--34 & & 39--46 &\\
 \citet{baraffe-et-al-2003} & & 6--7 & 8--10 & 10--11 & & 27--31 & & 37--43 &\\
 \citet{baraffe-et-al-2008}$^b$ & & & $\sim$9 & & & & & &\\
\hline
 \citet{baraffe-et-al-2003}$^d$ & & $\sim$7.5 & $\sim$10.5 & $\sim$11.5 & &
$\sim$38 & & $\sim$48 &\\
\hline
\end{tabular}
\begin{flushleft}
Remarks: All mass values were shortened to appropriate decimals and partly
rounded to halves or integers of a Jupiter mass. $^{a}$ Hot-start models. \\$^{b}$
Non irradiated models. $^{c}$ Using $M_{K{\rm s}}$ = 14.05~~$\pm$~~0.08 mag
\citep{marois-et-al-2008}. $^{d}$ Using $M_{K{\rm s}}\sim$~13.12 mag instead of
slightly different values $M_{K{\rm s}}$ = 13.13~~$\pm$~~0.08 mag for HR~8799~c and
$M_{K{\rm s}}$ = 13.11~$\pm$~0.12 mag
for HR~8799~d, given in \citet{marois-et-al-2008}.
\end{flushleft}
\end{table}