\begin{table}%T1
\caption{Best-fit parameters derived from RT-modelling of NGC~4013, NGC~5907 and NGC~4565 in the $V$-band.
$\tau_{V}^{f}$ is the visual optical depth when the galaxy is viewed face-on and $\theta$ is the inferred
inclination of the object. $h_{\rm d}$ and $z_{\rm d}$ are, respectively, the exponential scalelength and
exponential scaleheight of the dust assuming the distance listed in the second column. Distances to NGC~4013, NGC~4565
and NGC~5907 are taken, respectively, from Bottema (1995), Rupen (1991) and van~der~Kruit \& Searle (1982).  }
\label{tab_model}
%\centering
\par
\begin{tabular}{cccccc}
\hline
\hline
\\[-3mm]
Galaxy    & Distance & $\tau_{V}^{f}$ & $h_{\rm d}$ & $z_{\rm d}$ & $\theta$  \\
          &   (Mpc)  &                &  (kpc)  &  (kpc)  &   (deg)  \\ \hline
NGC~4013  &    12    &   0.67         &   2.45  &   0.13  &   89.7    \\
NGC~4565  &    10    &   0.63         &   9.7   &   0.21  &   88.0    \\
NGC~5907  &    11    &   0.49         &   5.29  &   0.11  &   87.2    \\ \hline
\end{tabular}
\end{table}