\begin{table}%t3
   %\centering
\par
\caption {\label{tab:fit}Fit parameters used to model the XTE J1814$-$338 optical spectrum (see Sect.~3.5 for details). Errors are at 90\% confidence level.}
\begin{tabular}{ccccccc}
\hline\hline
Model        &  $L_{\rm irr}$                        & Distance           &  $R_{\rm c}$           &  ${\eta}_*$      &  $R_{\rm in}$                    & ${\chi}^2$  \\ 
             &  (erg~s$^{-1}$)                   &   (kpc)            & ($R_{\odot}$)    &	            &  (cm)                        &             \\ 
\hline
Star         &  $(1.02 \pm 0.08)\times 10^{34}$  &  $11.75 \pm 0.54$  & $0.37 \pm 0.02$  & $0.16 \pm 0.07$  & $-$                            & 0.9   \\
Disc + star  &  $(2.74 \pm 0.03)\times 10^{34}$  &  $10.25 \pm 0.10$  & $0.34 \pm 0.01$  & $0.75 \pm 0.01$  & $< $$1.8 \times 10^{8}$ & $<$$ 0.8$   \\
\hline
\end{tabular}
\end{table}