Table 2:

Mean FIR luminosities of different AGN groups.

z
${L_{2-10~{\rm keV}}}$ $N_{\rm Det}/N$ Detected Stack All
  erg s-1   $\nu L_\nu$(60 $\mu$m rest), 1044 erg s-1
0.2-0.8 all 12/35 3.3 0.32 1.33 $\pm$ 0.31
0.8-1.4 all 22/83 11.3 1.43 4.04 $\pm$ 0.62
1.4-2.5 all 10/76 61.1 5.27 12.61 $\pm$ 3.12

0.2-0.8
<1042 4/16 1.9 0.09 0.55 $\pm$ 0.23
0.8-1.4 <1042 1/9 6.9 1.40 2.01 $\pm$ 0.91
1.4-2.5 <1042 0/1   3.92  

0.2-0.8
1042-43 2/12 4.4 0.60 1.23 $\pm$ 0.51
0.8-1.4 1042-43 7/37 12.3 1.56 3.60 $\pm$ 0.73
1.4-2.5 1042-43 6/18 63.4 4.35 24.04 $\pm$ 8.45

0.2-0.8
1043-44 6/7 3.8 1.91 3.54 $\pm$ 0.89
0.8-1.4 1043-44 13/32 10.5 1.61 5.22 $\pm$ 1.11
1.4-2.5 1043-44 3/51 69.3 5.30 9.06 $\pm$ 2.80

0.2-0.8
>1044 0/0      
0.8-1.4 >1044 1/5 18.2 2.32 5.50 $\pm$ 3.56
1.4-2.5 >1044 1/6 22.2 8.58 10.85 $\pm$ 4.77

z
${N_{\rm H}}$ $N_{\rm Det}/N$ Detected Stack All
  cm-2   $\nu L_\nu$(60 $\mu$m rest), 1044 erg s-1

0.8-1.4
<1022 2/10 13.7 1.12 4.15 $\pm$ 1.25
0.8-1.4 1022-23 6/25 11.6 1.47 3.89 $\pm$ 0.91
0.8-1.4 1023-24 10/28 9.6 1.76 4.57 $\pm$ 0.89
0.8-1.4 >1024 0/5   1.67 1.67 $\pm$ 0.88

Notes. Average FIR luminosities are given separately for the individual >$3\sigma$ detections, the stack of the nondetections, and the number-weighted mean for all sources. Errors for luminosities are standard deviations from bootstrapping and are dominated by the dispersion of the AGN population rather than measurement error.


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