The BeppoSAX High Energy Large Area Survey (HELLAS) has found so far 200 so
urces with a 5-10 flux higher than 5 x 10(-14) erg cm(-2) s(-1) in similar
to 80 deg(2) of sky. A summary on the optical identifications of a subsampl
e of these sources is presented here, Most of the identified sources are AG
N at 0.04 < z < 3.5. The fraction of sources showing absorption/extinction
in X-ray/optical to the total is 0.53 +/- 0.10, higher than in previous ROS
AT, and ASCA-ROSAT surveys, but in line with scenarios in which the bulk of
the hard Cosmic X-ray background (XRB) is made by highly obscured AGN (e.g
. Setti & Woltjer 1989, Comastri et al. 1995).