\begin{table}%t6
\caption{\label{tab:evolution}Parameters leading the total infrared LF evolution.}
\par
\small%\centerline
 {
\begin{tabular}{lccccc}
\hline \hline
{Authors} &Functional Form$^{{a}}$ &{Wavelength}&  & $\alpha_{L}$ & $\alpha_{\phi}$  \\
\hline
This study & DPL & 24 \& 70 $\mu$m & & $3.6\pm0.4$ & $-0.8\pm0.6$ \\
\citet{lefloch_2005} & DE & 24 $\mu$m &  & $\rm 3.2^{+0.7}_{-0.2}$ & $\rm 0.7^{+0.2}_{-0.6}$ \\
\citet{caputi_2007} & DE  & 24 $\mu$m & $z<1$ & $3.5\pm 0.4 $ & $-0.7\pm0.1$ \\
& & & $z>1$&$2.2\pm0.5$ & $-3.9\pm1.0$ \\
\citet{huynh_2007} & DPL  & 70 $\mu$m &  &$\rm 2.78^{+0.34}_{-0.32}$ & $0.0$ \\
\citet{hopkins_2004} & $\cdots$ & SFR compilation &  &$2.7\pm0.6$ & $0.15\pm0.6$\\
\hline
\end{tabular}}
\medskip
$^{{a}}$ DPL: Double Power Law; DE: Double Exponential. 
\end{table}