\begin{table}%t1
  %\centering
\par
\caption{\label{tab:parameters}Orbital and physical parameters of 2M0535-05.}
\par
\begin{tabular}{lc}
\hline \hline \noalign{\smallskip}
\multicolumn{1}{c}{P\textsc{roperty} }& O\textsc{bserved value}\\
\hline\noalign{\smallskip}
$a$, semi-major axis$^1$ & $0.0407 \pm 0.0008$~AU  \\
$e$, eccentricity$^1$ & $0.3216 \pm 0.0019$ \\
$P_{{\rm orb}}$, orbital period\tablefootmark{1} & $9.779556 \pm 0.000019$~d \\
$i$, orbital inclination to the line of sight\tablefootmark{1}  & $88.49 \pm 0.06^\circ$ \\
age\tablefootmark{1} & $1 \pm 0.5$~Myr \\
$T_{{\rm eff},1}$, primary effective temperature$^1$ & $2715 \pm 100$~K \\
$T_{{\rm eff},2}/T_{{\rm eff},1}$, effective temperature ratio$^1$ & $1.050 \pm 0.002$ \\
   $M_{1}$, primary mass$^1$ & $0.0572 \pm 0.0033~M_{\odot}$ \\
    $M_{2}$, secondary mass$^1$ & $0.0366 \pm 0.0022~M_{\odot}$ \\
    $R_{1}$, primary radius$^1$ & $0.690 \pm 0.011~R_{\odot}$ \\
    $R_{2}$, secondary radius$^1$ & $0.540 \pm 0.009~R_{\odot}$ \\
$L_{1}$, primary luminosity$^3$ & $8.9 \times 10^{24} \pm 3 \times 10^{24}$~W \\
$L_{2}$, secondary luminosity$^3$ & $6.6 \times 10^{24} \pm 2 \times 10^{24}$~W \\
    $P_{1}$, rotational period of the primary$^1$  & 3.293 $\pm 0.001$~d \\
    $P_{2}$, rotational period of the secondary$^1$ & 14.05 $\pm 0.05$~d \\
$ \bar{T}_{{\rm eff},1}$, modeled $T_{{\rm eff}}$ for the primary$^2$ & 2850~K\\
$ \bar{T}_{{\rm eff},2}$, modeled $T_{{\rm eff}}$ for the secondary$^2$ & 2700~K\\
    $ \bar{R}_1$, modeled radius for the primary$^2$ & $0.626~R_{\odot}$\\
    $ \bar{R}_2$, modeled radius for the secondary$^2$ & $0.44~R_{\odot}$\\
    \hline   
\end{tabular}
\tablefoot{\tablefoottext{1}{\citet{2009ApJ...699.1196G}.} \tablefoottext{2}{\citet{1998AetA...337..403B}.}
\tablefoottext{3}{Assuming an uncertainty of 200~K in $T_{{\rm eff},1}$ and $T_{{\rm eff},2}$.}}
\vspace*{4mm}
\end{table}