\begin{table}%t3
%%\centering
\par
\caption{\label{Table3}H$\alpha$- and IR-based star formation rates for the sample of ULIRGs.}
%\centerline
 {\small \begin{tabular}{lccccc}      
\hline \hline\noalign{\smallskip}
Galaxy & {$log(L_{\rm{IR}}$)}$^a$ & {$SFR(L(\rm{H}\alpha)_{\rm{obs}}$)}$^b$ & {$SFR(L(\rm{H}\alpha)_{\rm{med-ext}}$}$^c$) & {$SFR(L(\rm{H}\alpha)_{\rm{corr}}$)}$^d$& {$SFR(IR)$}$^e$\\ 
\hline
IRAS~13156+0435   & 12.13 & 5.5  & 26.2  & 23.7  & 232.9 \\
IRAS~18580+6527$^f$   & 12.26 & 17.1& 53.8  & 61.6  & 318.7 \\
IRAS~16007+3743   & 12.11 & 19.8 & 106.4 & 120.  & 222.5 \\
IRAS~06268+3509   & 12.51 & 3.7  & 22.1  & 95.6  & 493.5 \\
IRAS~08572+3915   & 12.17 & 3.6  & 16.7  & 12.2  & 255.5 \\
IRAS~14348-1447   & 12.39 & 20.2 & 263.1 & 301.0 & 424.1 \\
Arp~299$^{f}$     & 11.81 & 4.7  & 26.3  & 35.3  & 111.5 \\
IRAS~12112+0305   & 12.37 & 6.0  & 26.9  & 168.3 & 405.0 \\
Mrk~463$^{f}$     & 11.81 & 17.2 & 38.0  & 44.2  & 111.5 \\
IRAS~06487+2208   & 12.57 & 11.0 & 76.0  & 92.4  & 641.8 \\
IRAS~11087+5351$^{f}$ & 12.13 & 3.5  & 9.5   & 8.7   & 233.0 \\
Mrk~273$^{f}$     & 12.18 & --     &--       &  --     & 216.5 \\
IRAS~17208-0014   & 12.43 & 6.1  & --   & 126.5 & 465.0 \\
IRAS~15250+3609   & 12.09 & 2.5  & 19.7  & 69.1  & 212.5 \\
IRAS~12490-1009   & 12.07 & 2.0  & 6.4   & 9.5   & 203.0 \\
IRAS~14060+2919   & 12.18 & 6.4  & 24.3  & 35.5  & 261.5 \\
IRAS~15206+3342   & 12.27 & 135.7& 275.5 & 254.3 & 321.6 \\
\hline   
\end{tabular}}
\medskip
$^a$  IR luminosity derived following Sanders \& Mirabel (\cite{Sanders1996}); $^b$  SFR derived using the total observed H$\alpha$ flux given in Col.~2 of Table 2. Units are $M_\odot$~yr$^{-1}$; $^c$~SFR derived using the H$\alpha$ median extinction corrected values as specified in Table~\ref{Table2} Col.~6. Units are $M_\odot$~yr$^{-1}$; $^d$~SFR calculated using the two-dimensional extinction corrected H$\alpha$ luminosity as given in Table~\ref{Table2} Col.~5. Units are $M_\odot$~yr$^{-1}$; $^e$  SFR based on the IR-based luminosity values as given in Col.~2 of the present table. Units are $M_\odot$~yr$^{-1}$; $^f$~strong evidence for a Seyfert nucleus, for which we have not corrected this values.
\end{table}