  The Galactic Centre has been studied with the High Energy Stereoscopic System
(H.E.S.S.) for over 10 years, revealing a bright, complex gamma-ray morphology.
Besides a strong point-like very-high-energy gamma-ray source coincident with
the supermassive black hole Sgr A*, pre- vious analyses also revealed a diffuse
ridge of gamma-ray emission, indicative of a powerful cosmic-ray accelerator in
this region. The addition of a fifth telescope with 600 m 2 mirror area to the
centre of the H.E.S.S. array has increased the energy range accessible,
allowing observations to take place down to 100 GeV and potentially below. This
wider energy range allows an important overlap in observations with satellite
instruments such as the Fermi-LAT gamma-ray telescope. We will present the
results of new H.E.S.S observations of the Galactic Centre region and show a
detailed analysis of the central source, including comparisons to results at
other wavelengths.
