All Tables

Table 1: Mean spectral properties from the stacking analysis of sources in the 3 $\sigma$ hard sample detected in the pn at off-axis angle <11 $^\prime$ . $N_{\rm H}$ is fixed to the galactic value.
Table 2: Mean spectral properties from the stacking analysis of optically unobscured, optically obscured AGN and of the subclass of SFG objects. $N_{\rm H}$ is fixed to the galactic value.
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.
Table A.1: The 3 $\sigma$ hard sample: XMDS identifier and name, X-ray coordinates, X-ray flux (2-10 keV), hardness ratio between the 2-10 and 0.5-2 keV bands, distance between the X-ray and optical VVDS positions, VVDS B and I magnitudes, color classification, CFHTLS i' magnitude, SWIRE 3.6 and 24 $\mu$ m fluxes, spectroscopic and photometric redshifts, SED classification (see text) and absorption corrected X-ray luminosity. All magnitudes are in the AB system.
Table B.1: Spectral parameters obtained using simple power law model with both $\Gamma$ and $N_{\rm H}$ free parameters for sources for which $\chi ^2$ statistics can be used. The quoted errors correspond to the 90 per cent confidence level for one interesting parameter. The formal 0.00 errors on log $N_{\rm H}$ are the result of having fixed a minimum column density (the galactic value).
Table B.2: Spectral parameters obtained using a simple power law model with z = 0 and $\Gamma = 2.0$ in Cols. 2 and 3, $\Gamma = 1.7$ in Cols. 4 and 5 and using photometric (or spectroscopic when available) redshift in Cols. 6-8. In this case, the photon index is a free parameter when $\chi ^2$ statistics was used. The quoted errors correspond to the 90 per cent confidence level for one interesting parameter. The formal 0.00 errors on log $N_{\rm H}$ are the result of having fixed a minimum column density (the galactic value).