\begin{table}%t3
\caption{Parameter values of the fit of the mid-IR Luminosity Functions.
\label{tab3}}
        %\centerline
{\begin{tabular}{lccccccccc}
        \hline\hline
 & \multicolumn{3}{c}{{Type-1}} &\multicolumn{3}{c}{{Type-2}} & 
        \multicolumn{3}{c}{{All}} \\
 & {\scriptsize {${\rm \alpha}$}} & {\scriptsize  $\!\beta$}  
        & {\scriptsize  $\! {\rm log}~L_{15}^{*}$} & {\scriptsize $\alpha$} & {\scriptsize $\beta$} 
        & {\scriptsize ${\rm log}~L_{15}^*$} & {\scriptsize $\alpha$} &  {\scriptsize $\beta$} & 
        {\scriptsize ${\rm log}~L_{15}^*$} \\
\hline
\scriptsize{RMS}$^{a}$ & \scriptsize{0.0} & \scriptsize{2.1} & \scriptsize{42.8} & \scriptsize{0.0} & 
        \scriptsize{2.5} & \scriptsize{43.2} & \scriptsize{0.3} & \scriptsize{2.1} & \scriptsize{43.4} \\
\scriptsize{Xu03}$^{a, b}$ & -- &-- & -- & -- & -- & -- & {\scriptsize 0.3} & {\scriptsize 1.7} & {\scriptsize 43.4} \\
\scriptsize{Here}\scriptsize{(low-\textit{z})}$^{c}$ & {\scriptsize 1.3} & {\scriptsize 2.8} & 
        {\scriptsize 44.8} & {\scriptsize 0.9} & {\scriptsize 2.7} & {\scriptsize 44.1} & -- & -- & -- \\
\scriptsize{Here}\scriptsize{(int-\textit{z})}$^{c, d}$ & {\scriptsize 0.7} & {\scriptsize 2.8} & 
        {\scriptsize 45.4} & {\scriptsize 0.0} & {\scriptsize 2.7} & {\scriptsize 44.6} & -- & -- & -- \\
\hline
\end{tabular}}
\par
\smallskip
 $^{a}$ Luminosities have been converted to 15$~\mu$m using the 
		adopted SEDs.
 $^{b}$ From Xu et~al. (\cite{Xu03}).\\
 $^{c}$ Best fit solutions for type-1 (model "B'') and type-2 
		(Circinus SED, model "F'').\\
 $^{d}$ Intermediate redshift, $z=0.6$.
\par
\label{tbl:MidIR_LF_literature}
\end{table}