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Home All issues Volume 508 / No 2 (December III 2009) A&A, 508 2 (2009) L21-L25 Full HTML
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Table 1:

IR fluxes, star formation rates and derived dust attenuation.
z = 2.3
LAE_ $F_{24~\mu{\rm m}}$ $L_{\rm IR}$ $L_{\rm bol}$ ${\it SFR}_{\rm bol}$ A1600 Offset Remark
COSMOS_# $\mu$Jy erg s-1 erg s-1 $M_{\odot}$ yr-1   arcsec  
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  
z = 0.3
ID $F_{8~\mu{\rm m}}$ $L_{\rm IR}$ $L_{\rm bol}$ ${\it SFR}_{\rm bol}$ A1600 - Remark
  $\mu$Jy erg s-1 erg s-1 $M_{\odot}$ yr-1      
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 $ $5.07\pm0.05$    

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.

Source LaTeX | All tables | In the text

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