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The High Energy Stereoscopic System (H.E.S.S.) is an array of four imagingatmospheric-Cherenkov telescopes located in Namibia and designed to detectextensive air showers initiated by gamma-rays in the very-high-energy domain.It is an ideal instrument for surveying the Galactic plane in search of newsources, thanks to its location in the Southern Hemisphere, its excellentsensitivity, and its large field-of-view. The efforts of the H.E.S.S. GalacticPlane Survey, the first comprehensive survey of the inner Galaxy at TeVenergies, have contributed to the discovery of an unexpectedly large anddiverse population of over 60 sources of VHE gamma rays within its currentrange of l=250 to 65 degrees in longitude and |b|<=3.5 degrees in latitude. Thepopulation of VHE gamma-ray emitters is dominated by the pulsar wind nebula andsupernova remnant source classes, although nearly a third remain unidentifiedor confused.  The sensitivity of H.E.S.S. to sources in the inner Galaxy has improvedsignificantly over the past two years, from continued survey observations,dedicated follow-up observations of interesting source candidates, and from thedevelopment of advanced methods for discrimination of gamma-ray-induced showersfrom the dominant background of hadron-induced showers. The latest maps of theGalaxy at TeV energies will be presented, and a few remarkable new sources willbe highlighted.

Exploring the Galaxy at TeV energies: Latest results from the H.E.S.S. Galactic Plane Survey