Chandra and Spitzer observations of CDFS X-ray obscured QSOs

We present Chandra and Spitzer data of the 186, extragalactic, hard 2-10 keV X-ray selected sources, which lie in the central part of the Chandra Deep Field South (CDFS). For the vast majority of sources (99.5%) there is a spectroscopic or photometric redshift available. We classify 17 sources as X-ray obscured QSOs, according to strictly X-ray criteria, i.e. defined as having large hydrogen column densities (NH > 10 22 cm) and luminosities (Lx > 10 44 erg s). The surface density of X-ray obscured QSOs is ∼210 deg. We find 18 candidate Compton thick NH > 10 24 cmsources, of which three have QSO luminosities (Lx > 10 44 erg s). The X-ray obscured QSO comprise a mixed bag of objects, covering the redshift range z = 1.3− 4.3. Eight of these show narrow line optical spectra, two show no obscuration in their optical spectra presenting Broad Lines, while for the other seven there is only a photometric redshift available. About half of the X-ray obscured QSOs show high X-ray to optical flux ratios, X/O > 1, and red colours, I-3.6μm > 4. Combination of the X-ray with the mid-IR 8μm or 24μm flux can be used as an additional diagnostic to sift out the heavily obscured AGN. All X-ray selected QSOs present red mid-IR colours and can be easily separated among mid-IR sources, demonstrating that mid-IR selection provides a powerful tool for the detection of obscured QSOs.