\begin{table}%t1 
\caption{\label{tab:IR}IR fluxes, star formation rates and derived dust attenuation. }
\small%\centerline
{
\begin{tabular}{@{}lcccccccc}
\hline
\hline
\multicolumn{8}{c}{$z = 2.3$} \\
\hline
LAE\_ & $F_{24~\mu{\rm m}}$ & $L_{\rm IR}$ &  $L_{\rm bol}$ & ${\it SFR}_{\rm bol}$ & $A_{1600}$ & Offset & Remark \\
COSMOS\_\# & $\mu$Jy & erg s$^{-1}$ & erg s$^{-1}$ & $M_{\odot}$ yr$^{-1}$ & & arcsec &  &  \\
\hline
  20 & $154\pm16$ &  $46.50\pm0.05$ &  $46.50\pm0.07$ & $     1420\pm220$   & $5.51\pm0.18$ & 0.02 & AGN \\
  36 & $835\pm20$ &  $47.69\pm0.02$ &  $47.69\pm0.02$ & $   21830\pm1000$ & $7.65\pm0.05$ & 0.02 & AGN \\
\hline
\multicolumn{8}{c}{$z = 0.3$} \\
\hline
ID & $F_{8~\mu{\rm m}}$   &  $L_{\rm IR}$ &  $L_{\rm bol}$ & ${\it SFR}_{\rm bol}$ & $A_{1600}$ & --  & Remark & \\
    & $\mu$Jy & erg s$^{-1}$ & erg s$^{-1}$ & $M_{\odot}$ yr$^{-1}$ &  &  \\
\hline
CDFS\_1348 & $1.63\pm0.03$   & $45.19\pm0.01$ & $45.20\pm0.01$ & $70.9\pm2.1$   & $4.91\pm0.03$ &  & \\
CDFS\_1821 & $0.38\pm0.05$   & $44.17\pm0.08$ & $44.20\pm0.09$ &$7.1\pm1.4$      & $2.69\pm0.21$ & &   Unclass. & \\
\hline
\end{tabular}}
\smallskip
  Columns are: (1)~flux in the 8/24~$\mu$m data; (2)~infrared luminosity; (3)~bolometric luminosity; (4)~star formation rate; (5)~dust attenuation derived from the infrared luminosities; (6)~offsets between MIPS catalogue source and LAE candidate in z23~sample; and~(7)~other remarks. The IDs for the z03 sample are from Deharveng et~al.~(\cite{Deharveng2008}). Full table is available in the online version. 
\end{table}