American Astronomical Society, Astrophysical Journal, 1(738), p. 44, 2011
DOI: 10.1088/0004-637x/738/1/44
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ApJ in press: 15 pages, 6 figures, 3 tables ; International audience ; We use the 4Ms CDF-S survey to place direct X-ray constraints on the ubiquity of z~2 heavily obscured AGNs in K10 keV observatories. On the basis of these analyses we estimate the space density for typical (intrinsic X-ray luminosities of L_X>1E43 erg/s) heavily obscured and Compton-thick AGNs at z~2. Our space-density constraints are conservative lower limits but they are already consistent with the range of predictions from X-ray background models.