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Observations of the Galactic Plane performed by the H.E.S.S. telescope arrayhave revealed a significant excess at very-high-energies (VHE; E>0.1 TeV) fromthe direction of PSR J1459-60, a rather old gamma-ray pulsar (64 kyr) with aspindown energy of ~10^36 erg/s, discovered by the Fermi/LAT satellite inhigh-energy (HE) gamma-rays. The X-ray pulsar counterpart has been recentlydetected using the Suzaku satellite. In this contribution, we present thediscovery of a new VHE gamma-ray source, including morphological and spectralanalyses. Its association with the gamma-ray pulsar in a PWN scenario will bediscussed.

A newly discovered VHE gamma-ray PWN candidate around PSR J1459-60