\begin{table}%T6 
  \caption{\label{radiofirt}Additional \FIR\ and radio properties.}
  \small%\centering
\par
 \begin{tabular}{l  cr  c }
\hline\hline   
   \noalign{\smallskip}
Galaxy        &   $q$\tablefootmark{a}   &     $\log R$\tablefootmark{b}         &  $\tau_{\rm g}$ \\ 
              &           &                     &  [Gyr] \\  
\hline   
\par
HCG 31 AC       & 2.39  &  1.19    & 1.92   \\ 
HCG 31 B        &\nodata&  1.25    &  5.3   \\
HCG 31 F        &\nodata&  \nodata & 2.9   \\ 
HCG 31 G        &\nodata&  1.11    & 2.3    \\
Mkn 1087        & 2.53  &  1.30    & 3.3    \\
Haro 15         & 2.01  &  1.48    & 1.9    \\
Mkn 1199        & 2.39  &  1.31    & 0.40   \\
Mkn 5           &\nodata&  \nodata & 2.1   \\ 
IRAS~08208+2816 & 2.01  &  1.57    & \nodata\\
IRAS~08339+6517 & 2.33  &  1.21    & 0.89   \\
POX 4           & 2.25  &  0.93    & 4.2    \\
UM 420          & 2.71  &  1.08    & \nodata\\
SBS~0926+606    & 2.18  &  0.79    & 2.0 (A), 5.6 (B)    \\ 
SBS~0948+532    &\nodata& \nodata  & \nodata\\  
SBS~1054+365    & 2.79  & $-$0.10  & 4.0    \\  
SBS~1211+540    &\nodata& \nodata  & 3.5  \\ 
SBS~1319+579    & 2.15  & \nodata  & 12.7   \\  
SBS~1415+437    &\nodata& \nodata  &  3.5   \\ 
III~Zw~107      & 2.34  &  1.06    &  3.5   \\ 
Tol 9           & 2.03  &  1.16    &  1.95  \\ 
Tol 1457-262    & 2.00  &  1.43    &  1.51  \\ 
Arp 252         & 1.69  &  2.28    & \nodata\\ 
NGC 5253        & 2.62  &  0.33    &  0.97  \\ 
 \hline   
  \end{tabular}
 \tablefoot{\tablefoottext{a}{The logarithmic ratio of \FIR\ to radio flux density parameter, $q$, is defined in Eq.~(\ref{agnq}).}\\
  \tablefoottext{b}{$R$ is the nonthermal to thermal ratio, derived from the 1.4~GHz and \Ha\ fluxes.}\\
  \tablefoottext{c}{The gas depletion timescale is defined as $\tau_{\rm g}=1.32$\MHi/\SFR\  (Skillman et~al. \cite{Skillman2003}).}}
\end{table}