2007

Localising the H.E.S.S. Galactic Centre point source

van Eldik, C., Bolz, O., Braun, I. et al.

Understand

Observations by the H.E.S.S.

system of imaging atmospheric Cherenkov telescopes provide the most sensitive measurements of the Galactic Centre region in the energy range 150 GeV - 30 TeV.
The vicinity of the kinetic centre of our galaxy harbours numerous objects which could potentially accelerate particles to very high energies (VHE, > 100 GeV) and thus produce the Gamma-ray flux observed.
Within statistical and systematic errors, the centroid of the point-like emission measured by H.E.S.S.

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