\begin{table}%t1
\caption{\label{table0}The stellar mass fraction $f_{\ast}(t)$ after gas recycling, as~a~function of population age for different IMFs of power-law form (${\rm d}n/{\rm d} \log M \propto M^{-m}$), and the~$L_{\rm IR}$ to $\it SFR$ calibration.}    
%\centering
\par
\begin{tabular}{ c c c c c c c}         
\hline  \hline  \noalign{\smallskip}
age      & Scalo & Kroupa   & Salpeter  & Top-heavy 1 & Top-heavy 2 & Top-heavy 3 \\
 Gyr    & (1986)& (1993)   & $m=1.35$  & $m=1.15$  & $m=1.0$   & $m=0.85$   \\     
\hline                                                 
  0.01   &   0.98     &   0.97   &   0.90    & 0.87 &   0.83  	&   0.60                \\
  0.05   &   0.94     &   0.92   &   0.85    & 0.74 &   0.62  	&   0.53                \\
  0.1    &   0.92     &   0.90   &   0.83    & 0.70 &   0.58  	&   0.44                \\ 
  1.0    &   0.86     &   0.81   &   0.75    & 0.61 &   0.48  	&   0.35                \\
  3.0    &   0.80     &   0.75   &   0.72    & 0.57 &   0.44  	&   0.32                \\ 
  7.0    &   0.75     &   0.72   &   0.70    & 0.56 &   0.42  	&   0.31                \\
  10.    &   0.73     &   0.70   &   0.65    & 0.55 &   0.41  	&   0.30                \\
  15.    &   0.71     &   0.69   &   0.65    & 0.54 &   0.40  	&   0.30                \\
\hline  \noalign{\smallskip}
$\frac{{\it SFR}\ [M_\odot/{\rm yr}]}{L_{\rm IR}/L_\odot}$ & $3.3 \times 10^{-10}$ & $2.2 \times 10^{-10}$ & $1.63 \times 10^{-10}$ & $1.01 \times 10^{-10}$ & $0.63 \times 10^{-10}$ & $0.46 \times 10^{-10}$ \\[3pt]
\hline 
\end{tabular}
\vspace*{5mm}
\end{table}