  Recent X-ray surveys with Chandra and XMM-Newton have found several genuine
Type II quasars, the long sought-after population of high-luminosity
(high-redshift) Seyfert 2 galaxies, and a sizable number of Type II quasar
candidates. However, at present it is hard to know whether the on-going X-ray
surveys are providing a reliable and nearly complete census of the Type II
quasar population. In order to address this open issue and shed light on the
broad-band properties of Type II quasars, we used the sample of 291
high-ionization narrow emission-line AGN at z=0.3-0.83 selected from the Sloan
Digital Sky Survey by Zakamska et al. (2003). Using archival X-ray information,
we were able to place constraints on the X-ray emission of 17 of these objects
(three X-ray detections and 14 upper limits). Using the [O III]5007 line
luminosities to predict the intrinsic X-ray power of the AGN, we found that at
least 47% of the objects in the observed sample provides evidence for the
presence of X-ray absorption (with N_H>10^22 cm^-2), including the four highest
luminosity sources with predicted unobscured luminosities of ~10^45 erg/s. For
the only source with moderate-quality XMM-Newton spectral data, all of the
pieces of the puzzle (2-10 keV luminosity of ~4x10^44 erg/s, N_H~1-3x10^22
cm^-2, and unobscured magnitude M_B=-26 assure that this is a genuine Type II
quasar.
