Table 3: Total number of sources, number of optically unobscured and optically obscured AGN, number of X-ray absorbed AGN ( $N_{\rm H} > 10^{22}$ cm-2), and number of optically unobscured and obscured AGN among X-ray absorbed AGN in each X-ray flux, redshift and absorption corrected X-ray luminosity bin (see text and Fig. 21). Fluxes are in erg cm-2 s-1, luminosities are in erg s-1.
Bins       $N_{\rm H} > 10^{22}$
  $N_{\rm tot}$ Opt. Unobsc. Opt. Obsc. $N_{\rm abs}$ Opt. Unobsc. Opt. Obsc.
$-14 < \mbox{log}~F_{2-10} < -13.75$ 27 5 22 17 2 15
$-13.75 < \mbox{log}~F_{2-10} < -13.5$ 61 20 41 32 8 24
$-13.5 < \mbox{log}~F_{2-10} < -13.25$ 25 11 14 9 2 7
$-13.25 < \mbox{log}~F_{2-10} < -12.5$ 9 3 6 2 0 2
z < 0.5 28 2 26 13 0 13
0.5 < z < 1 42 11 31 14 1 13
1 < z < 1.5 21 5 16 15 3 12
1.5 < z < 2 11 6 5 6 1 5
z > 2 20 15 5 12 7 5
log  L2-10 < 42.5 5 0 5 2 0 2
$42.5 < \mbox{log}~L_{2-10} < 43.5$ 27 1 26 15 0 15
$43.5 < \mbox{log}~L_{2-10} < 44.5$ 54 15 39 23 4 19
log  L2-10 > 44.5 36 23 13 20 8 12


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