\begin{table}%T3
\caption{Dust components derived from SED fitting of NGC~4013, NGC~5907 and NGC~4565 in the FIR/submm/mm
regime. We decompose the spectrum into 2 components; warm dust of temperature $T^{\rm W}$ and cold dust of 
temperature $T^{\rm C}$. The ratio of cold dust mass to warm dust mass is given as $\frac{M^{\rm C}}{M^{\rm W}}$. An index of 1.5 has 
been assumed for the wavelength dependency of the emissivity ($Q\propto \lambda^{-1.5}$).}
\label{tab_sed}
%\centering
\par
\begin{tabular}{cccc}
\hline
\hline\\[-3mm]
Galaxy    &    $T^{\rm W}$ & $T^{\rm C}$ &  $\frac{M^{\rm C}}{M^{\rm W}}$  \\
          &     (K)    &  (K)    &                         \\ \hline
NGC~4013  &      39    &  23     &         49              \\
NGC~4565  &      43    &  20     &         99              \\
NGC~5907  &      28    &  13     &         5.7             \\ \hline
\end{tabular}
\end{table}