  Combining the results of targeted observations, H.E.S.S. has accumulated a
large amount of extra-galactic exposure at TeV energies. Due to its large field
of view a considerable part of the sky (0.6 sr) has been observed with high
sensitivity outside the targeted observation positions. Since this exposure
region contains little inherent bias, it is well suited for studies of
extra-galactic source populations. Given the correlation between ultra-high
energy cosmic rays and nearby extra-galactic objects recently claimed by the
Auger collaboration, this unbiased sky sample by H.E.S.S. is of interest since
it includes (besides the targeted sources) 63 AGN within 100 Mpc, for which
very-high energy gamma-ray flux limits are derived.
