The H.E.S.S. Imaging Atmospheric Cherenkov Telescope Array is currently the
most sensitive instrument for Very High Energy (VHE) gamma-ray observations in
the energy range of about 0.1-10 TeV. During more than two years of operation
with the complete 4-telescope array, many galactic and extragalactic VHE
gamma-ray sources have been discovered. With its superior sensitivity and its
large field-of-view camera, H.E.S.S. is particularly suited for surveys and
detailed studies of extended sources. A selection of recent H.E.S.S. results is
presented in this proceeding.Comment: 8 pages, 4 figures, to appear in the proceedings of the 41st
Rencontres de Moriond on Electroweak Interactions and Unified Theories, La
Thuile, Aosta Valley, Italy, 11-18 March 200
