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2HWC J1928+177 is a source recently discovered at TeV energies in the secondHAWC catalog. It is coincident with the Fermi unidentified source 3FGLJ1928+1739 and the pulsar PSR J1928+1746, which is 83 kyr old and located at adistance of 5 kpc with an Edot=1.6 x 10$^{36}$ erg/s. 2HWC J1928+177 is notdetected by any of the IACTs currently in operation, which puts strongconstrains on the morphology and spectrum of the source. There is no sign ofshell-like structure in the region at other wavelengths, which in addition tothe presence of a pulsar at the center, points to a Pulsar Wind Nebula originof the TeV emission. We present a dedicated morphological and spectral analysisof the region using HAWC and H.E.S.S. data to unveil the nature of the sourceand study its properties.

Morphological and spectral measurements of 2HWC J1928+177 with HAWC and H.E.S.S