Optical positions relative to the International
Reference Stars Catalogue (IRS), and therefore in the system
of the FK5, have been obtained for the optical counterparts
of 40 compact extragalactic radio sources south
of +6 . Many of these sources are being considered
as possible Benchmark objects for the establishment
of a quasi−inertial uni ed radio/optical reference frame.
Precision levels as good as 0.100 in both coordinates were
achieved. A comparison with VLBI radio positions available
for these sources is presented. We give new evidence
for the existence of an o set in the origin of right ascension
between the radio and optical reference frames as de ned
at present.