\begin{table} \caption{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 $ & $5.51\pm0.18$ & 1.49 & AGN \\ 36 & $835\pm20$ & $47.69\pm0.02$ & $47.69\pm0.02$ & $ 21830\pm1000 $ & $7.65\pm0.05$ & 0.19 & AGN \\ 42 & $155\pm47$ & $46.50\pm0.13$ & $46.51\pm0.19$ & $ 1460\pm510 $ & $3.89\pm0.45$ & 0.82 & AGN \\ 52 & $289\pm41$ & $46.94\pm0.08$ & $46.94\pm0.10$ & $ 3920\pm780 $ & $6.90\pm0.24$ & 0.56 & AGN \\ 94 & $132\pm87$ & $46.39\pm0.19$ & $46.39\pm0.38$ & $ 1100\pm640 $ & $7.13\pm0.95$ & 1.28 & \\ 96 & $88\pm46$ & $46.10\pm0.17$ & $46.11\pm0.30$ & $ 570\pm390 $ & $5.03\pm0.74$ & 3.83 & \\ 101 & $259\pm17$ & $46.86\pm0.04$ & $46.86\pm0.06$ & $ 3280\pm440 $ & $7.31\pm0.16$ & 0.09 & AGN \\ 108 & $143\pm18$ & $46.44\pm0.07$ & $46.45\pm0.08$ & $ 1270\pm230 $ & $3.96\pm0.21$ & 0.39 & AGN \\ 115 & $202\pm16$ & $46.69\pm0.05$ & $46.69\pm0.05$ & $ 2210\pm260 $ & $4.83\pm0.13$ & 0.06 & AGN \\ 126 & $181\pm25$ & $46.61\pm0.08$ & $46.62\pm0.09$ & $ 1880\pm360 $ & $3.73\pm0.22$ & 0.44 & AGN \\ 129 & $182\pm14$ & $46.61\pm0.05$ & $46.62\pm0.06$ & $ 1860\pm230 $ & $5.91\pm0.14$ & 0.29 & AGN \\ 130 & $75\pm11$ & $45.99\pm0.08$ & $46.00\pm0.11$ & $ 450\pm100 $ & $5.45\pm0.27$ & 0.56 & AGN \\ 140 & $509\pm19$ & $47.34\pm0.02$ & $47.34\pm0.03$ & $ 9790\pm670 $ & $7.36\pm0.08$ & 0.15 & AGN \\ 150 & $297\pm16$ & $46.96\pm0.03$ & $46.96\pm0.05$ & $ 4090\pm420 $ & $7.12\pm0.12$ & 0.35 & AGN \\ 151 & $404\pm11$ & $47.18\pm0.02$ & $47.18\pm0.04$ & $ 6740\pm610 $ & $8.01\pm0.10$ & 0.45 & AGN \\ 152 & $90\pm13$ & $46.12\pm0.08$ & $46.13\pm0.10$ & $ 610\pm120 $ & $3.95\pm0.23$ & 2.73 & \\ 155 & $190\pm11$ & $46.64\pm0.04$ & $46.66\pm0.04$ & $ 2040\pm180 $ & $3.79\pm0.10$ & 0.37 & AGN \\ 162 & $111\pm11$ & $46.26\pm0.06$ & $46.26\pm0.11$ & $ 830\pm180 $ & $6.69\pm0.27$ & 2.75 & \\ 167 & $216\pm18$ & $46.73\pm0.05$ & $46.74\pm0.06$ & $ 2440\pm340 $ & $6.66\pm0.16$ & 3.09 & \\ 171 & $123\pm11$ & $46.34\pm0.05$ & $46.34\pm0.06$ & $ 990\pm130 $ & $4.61\pm0.15$ & 0.70 & \\ 173 & $197\pm14$ & $46.67\pm0.04$ & $46.68\pm0.05$ & $ 2130\pm220 $ & $4.75\pm0.12$ & 1.05 & AGN \\ 175 & $277\pm16$ & $46.91\pm0.04$ & $46.91\pm0.05$ & $ 3660\pm400 $ & $7.13\pm0.13$ & 0.44 & AGN \\ 179 & $352\pm190$ & $47.08\pm0.18$ & $47.08\pm0.31$ & $ 5390\pm2750 $ & $7.83\pm0.77$ & 0.25 & \\ 183 & $95\pm11$ & $46.16\pm0.07$ & $46.16\pm0.08$ & $ 660\pm110 $ & $4.80\pm0.20$ & 0.81 & \\ 187 & $82\pm11$ & $46.05\pm0.07$ & $46.05\pm0.09$ & $ 510\pm100 $ & $4.41\pm0.22$ & 2.62 & \\ \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 & $1.63\pm0.03$ & $45.19\pm0.01$ & $45.20\pm0.01$ & $ 71\pm2 $ & $4.91\pm0.03$ & & & \\ CDFS\_1821 & $0.38\pm0.05$ & $44.17\pm0.08$ & $44.20\pm0.09$ & $ 7\pm1 $ & $2.69\pm0.21$ & & & \\ CDFS\_2422 & $10.72\pm0.04$ & $46.52\pm0.01$ & $46.52\pm0.01$ & $ 1480\pm10 $ & $7.52\pm0.01$ & & Unclass. & \\ CDFS\_3801 & $0.64\pm0.06$ & $44.53\pm0.06$ & $44.54\pm0.07$ & $ 16\pm2 $ & $3.57\pm0.16$ & & & \\ CDFS\_4927 & $0.70\pm0.03$ & $44.60\pm0.03$ & $44.61\pm0.03$ & $ 18\pm1 $ & $4.14\pm0.08$ & & & \\ CDFS\_5007 & $0.46\pm0.09$ & $44.31\pm0.09$ & $44.32\pm0.12$ & $ 9\pm2 $ & $3.45\pm0.28$ & & & \\ CDFS\_5448 & $1.56\pm0.05$ & $45.16\pm0.02$ & $45.16\pm0.02$ & $ 66\pm3 $ & $5.20\pm0.05$ & & & \\ CDFS\_6523 & $1.34\pm0.04$ & $45.05\pm0.02$ & $45.06\pm0.02$ & $ 51\pm2 $ & $4.98\pm0.05$ & & & \\ CDFS\_6535 & $2.36\pm0.05$ & $45.45\pm0.01$ & $45.46\pm0.01$ & $ 130\pm4 $ & $5.44\pm0.04$ & & & \\ CDFS\_7100 & $1.27\pm0.06$ & $45.01\pm0.03$ & $45.02\pm0.03$ & $ 47\pm3 $ & $4.87\pm0.08$ & & & \\ CDFS\_16104 & $0.33\pm0.06$ & $44.07\pm0.09$ & $44.13\pm0.12$ & $ 6\pm2 $ & $2.12\pm0.25$ & & & \\ CDFS\_17033 & $0.44\pm0.07$ & $44.28\pm0.08$ & $44.29\pm0.10$ & $ 8\pm2 $ & $3.38\pm0.23$ & & & \\ CDFS\_19355 & $5.33\pm0.06$ & $46.02\pm0.01$ & $46.03\pm0.01$ & $ 478\pm8 $ & $6.02\pm0.02$ & & Unclass. & \\ CDFS\_21667 & $3.54\pm0.05$ & $45.74\pm0.01$ & $45.74\pm0.01$ & $ 246\pm6 $ & $5.79\pm0.03$ & & & \\ CDFS\_21739 & $0.78\pm0.05$ & $44.67\pm0.04$ & $44.69\pm0.04$ & $ 22\pm2 $ & $3.73\pm0.10$ & & Unclass. & \\ CDFS\_30899 & $0.37\pm0.04$ & $44.15\pm0.06$ & $44.18\pm0.07$ & $ 7\pm1 $ & $2.78\pm0.16$ & & & \\ ELAISS1\_13715 & $2.90\pm0.20$ & $45.60\pm0.04$ & $45.60\pm0.05$ & $ 179\pm18 $ & $5.51\pm0.11$ & & Unclass. & \\ ELAISS1\_16998 & $4.75\pm0.07$ & $45.94\pm0.01$ & $45.95\pm0.01$ & $ 396\pm9 $ & $6.64\pm0.02$ & & & \\ ELAISS1\_6587 & $0.26\pm0.06$ & $43.89\pm0.10$ & $43.94\pm0.14$ & $ 4\pm1 $ & $2.30\pm0.30$ & & AGN & \\ ELAISS1\_8180 & $17.72\pm0.04$ & $46.87\pm0.01$ & $46.87\pm0.01$ & $ 3340\pm10 $ & $7.82\pm0.01$ & & Unclass. & \\ ELAISS1\_21062 & $0.36\pm0.10$ & $44.13\pm0.13$ & $44.17\pm0.18$ & $ 7\pm2 $ & $2.54\pm0.39$ & & & \\ ELAISS1\_23257 & $0.42\pm0.05$ & $44.23\pm0.06$ & $44.26\pm0.07$ & $ 8\pm1 $ & $2.68\pm0.17$ & & Unclass. & \\ ELAISS1\_23425 & $0.17\pm0.05$ & $43.62\pm0.12$ & $43.78\pm0.18$ & $ 3\pm1 $ & $1.16\pm0.27$ & & & \\ ELAISS1\_16921 & $1.93\pm0.05$ & $45.31\pm0.02$ & $45.31\pm0.02$ & $ 93\pm4 $ & $5.07\pm0.05$ & & & \\ \hline %\label{tab:IR} \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. (2008). Full table is available in the online version. \end{table}